https://luna.uai.it/index.php?title=Alta_risoluzione&feed=atom&action=historyAlta risoluzione - Cronologia2024-03-28T12:42:31ZCronologia della pagina su questo sitoMediaWiki 1.17.0https://luna.uai.it/index.php?title=Alta_risoluzione&diff=421&oldid=prevAntonio: Pagina svuotata2012-02-16T20:12:56Z<p>Pagina svuotata</p>
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<td colspan='2' style="background-color: white; color:black;">← Versione meno recente</td>
<td colspan='2' style="background-color: white; color:black;">Versione delle 20:12, 16 feb 2012</td>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">Questo settore del sito è dedicato alle immagini in alta risoluzione della Luna, che fanno parte di quelle riprese fotografiche effettuate a più alto ingrandimento dei dettagli della superficie lunare.<br>Il campo di lavoro degli osservatori lunari in questo contesto è vastissimo, avendo a disposizione esattamente la metà (e talvolta anche una quantità di superficie maggiore durante le condizioni favorevoli di librazione) della superficie totale lunare, ed inoltre in tutte le condizioni possibili di luce che si verificano durante il susseguirsi delle fasi lunari. Le tecniche di ripresa possono essere molteplici, partendo dalla tradizionale macchina fotografica a pellicola per i fotografi di tipo tradizionale (per la verità ormai molto rari), per poi passare alle moderne macchine digitali che ormai hanno pressocchè sostituito le precedenti, oppure effettuando le riprese con webcam adattate allo scopo o con altri strumenti di ripresa di moderna concezione, per concludere con lo strumento principe per la fotografia astronomica e cioè la camera CCD, strumento idoneo per le riprese ad alta risoluzione e appositamente ideato per la ricerca scientifica di tutti i generi in astronomia. Ovviamente questi strumenti di ripresa devono essere collegati a telescopi astronomici dotati di montatura equatoriale motorizzata che deve essere ben stazionata al polo celeste, perchè possa ottimamente seguire la Luna nel suo moto nel cielo, ed è necessario inoltre inserire anche degli elementi ottici che possano aumentare la lunghezza focale dello strumento usato come le lenti di Barlow. Data la vicinanza del nostro satellite si può ottenere dei buoni risultati usando anche strumenti di piccole dimensioni. </del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.12a bru.jpg|center|640x480px|Fig.12a bru.jpg]]&nbsp;&nbsp;&nbsp; Fig.12 - Il cratere Moltke, immagine di Bruno Cantarella (AL) , telescopio con webcam ed elaborazione con Registax 6&nbsp;<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.11a sep.jpg|center|746x417px|Fig.11a sep.jpg]]&nbsp;Fig.11 - Il cratere Copernico ripreso in diverse condizioni di luce, a sinistra da Sergio Saltamonti (LI) e Paolo Lazzarotti (MS)<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.10a ant.jpg|center|592x501px|Fig.10a ant.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.10 - Il cratere Stadius, immagine di Antonio Marino (NA) , i dati tecnici sono specificati sopra<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.9a val.jpg|center|578x486px|Fig.9a val.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.9 - Il cratere Maurolycus, immagine di Valerio Fontani (FI), i dati tecnici sono specificati sopra<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.8a ser.jpg|center|631x469px|Fig.8a ser.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.8 - I crateri Theophilus, Cyrillus e Catharina, immagine di Sergio Saltamonti (LI)<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.7a bru.jpg|center|Fig.7a bru.jpg]]&nbsp;&nbsp;&nbsp;&nbsp; Fig.7 - Il cratere Gutenberg, immagine di Bruno Cantarella (AL), telescopio MTO&nbsp;100/1000, Barlow 2X&nbsp;Apo con webcam<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.6a ser.jpg|center|625x467px|Fig.6a ser.jpg]]&nbsp;&nbsp; Fig.6 - Il cratere Clavius, immagine di Sergio Saltamonti (LI), telescopio OTA&nbsp;Meade 10", Barlow 3X, camera Skynix 2.1C<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.5a cla.jpg|center|Fig.5a cla.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.5 - Mons e Gamma Piton, immagine di Claudio Vantaggiato (FG), elaborazione con Registax 5&nbsp;<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.3a mau.jpg|center|635x481px|Fig.3a mau.jpg]]&nbsp; Fig.3 - Il polo Sud lunare, immagine di Maurizio e Francesca Cecchini (Montalcino, SI) i dati tecnici sono specificati sopra<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.2a mau.jpg|center|650x488px|Fig.2a mau.jpg]]&nbsp; Fig.2 - La zona del cratere Plato, immagine di Maurizio e Francesca Cecchini (Montalcino, SI) i dati sono specificati sopra<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== [[Image:Fig.1a mar.JPG|center|Fig.1a mar.JPG]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Fig.1 - Il cratere Copernico, immagine di Marco Vedovato (Predazzo, TN) i dati tecnici sono specificati sopra&nbsp;<br> =====</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;"></del></div></td><td colspan="2"> </td></tr>
<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">===== &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Sezione di Ricerca Luna  =====</del></div></td><td colspan="2"> </td></tr>
</table>Antoniohttps://luna.uai.it/index.php?title=Alta_risoluzione&diff=368&oldid=prevAntonio il 19:30, 25 gen 20122012-01-25T19:30:43Z<p></p>
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<td colspan='2' style="background-color: white; color:black;">Versione delle 19:30, 25 gen 2012</td>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div>===== [[Image:Fig.12a bru.jpg|center|640x480px|Fig.12a bru.jpg]]<del class="diffchange diffchange-inline">&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;</del>&nbsp;&nbsp;&nbsp; Fig.12 - Il cratere Moltke, immagine di Bruno Cantarella, telescopio con webcam ed elaborazione con Registax 6&nbsp;<br> =====</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>===== [[Image:Fig.12a bru.jpg|center|640x480px|Fig.12a bru.jpg]]&nbsp;&nbsp;&nbsp; Fig.12 - Il cratere Moltke, immagine di Bruno Cantarella <ins class="diffchange diffchange-inline">(AL) </ins>, telescopio con webcam ed elaborazione con Registax 6&nbsp;<br> =====</div></td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div>===== [[Image:Fig.10a ant.jpg|center|592x501px|Fig.10a ant.jpg]]<del class="diffchange diffchange-inline">&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;</del>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.10 - Il cratere Stadius, immagine di Antonio Marino, i dati tecnici sono specificati sopra<br> =====</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>===== [[Image:Fig.10a ant.jpg|center|592x501px|Fig.10a ant.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.10 - Il cratere Stadius, immagine di Antonio Marino <ins class="diffchange diffchange-inline">(NA) </ins>, i dati tecnici sono specificati sopra<br> =====</div></td></tr>
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</table>Antoniohttps://luna.uai.it/index.php?title=Alta_risoluzione&diff=288&oldid=prevAntonio il 22:40, 30 nov 20112011-11-30T22:40:42Z<p></p>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">== Pagina in costruzione<br> ==</del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;">'''<u>N.B. IL SITO SARA' UFFICIALMENTE ON-LINE IL 1 DICEMBRE PROSSIMO</u>''' </del></div></td><td colspan="2"> </td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Questo settore del sito è dedicato alle immagini in alta risoluzione della Luna, che fanno parte di quelle riprese fotografiche effettuate a più alto ingrandimento dei dettagli della superficie lunare.<br>Il campo di lavoro degli osservatori lunari in questo contesto è vastissimo, avendo a disposizione esattamente la metà (e talvolta anche una quantità di superficie maggiore durante le condizioni favorevoli di librazione) della superficie totale lunare, ed inoltre in tutte le condizioni possibili di luce che si verificano durante il susseguirsi delle fasi lunari. Le tecniche di ripresa possono essere molteplici, partendo dalla tradizionale macchina fotografica a pellicola per i fotografi di tipo tradizionale (per la verità ormai molto rari), per poi passare alle moderne macchine digitali che ormai hanno pressocchè sostituito le precedenti, oppure effettuando le riprese con webcam adattate allo scopo o con altri strumenti di ripresa di moderna concezione, per concludere con lo strumento principe per la fotografia astronomica e cioè la camera CCD, strumento idoneo per le riprese ad alta risoluzione e appositamente ideato per la ricerca scientifica di tutti i generi in astronomia. Ovviamente questi strumenti di ripresa devono essere collegati a telescopi astronomici dotati di montatura equatoriale motorizzata che deve essere ben stazionata al polo celeste, perchè possa ottimamente seguire la Luna nel suo moto nel cielo, ed è necessario inoltre inserire anche degli elementi ottici che possano aumentare la lunghezza focale dello strumento usato come le lenti di Barlow. Data la vicinanza del nostro satellite si può ottenere dei buoni risultati usando anche strumenti di piccole dimensioni.  </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Questo settore del sito è dedicato alle immagini in alta risoluzione della Luna, che fanno parte di quelle riprese fotografiche effettuate a più alto ingrandimento dei dettagli della superficie lunare.<br>Il campo di lavoro degli osservatori lunari in questo contesto è vastissimo, avendo a disposizione esattamente la metà (e talvolta anche una quantità di superficie maggiore durante le condizioni favorevoli di librazione) della superficie totale lunare, ed inoltre in tutte le condizioni possibili di luce che si verificano durante il susseguirsi delle fasi lunari. Le tecniche di ripresa possono essere molteplici, partendo dalla tradizionale macchina fotografica a pellicola per i fotografi di tipo tradizionale (per la verità ormai molto rari), per poi passare alle moderne macchine digitali che ormai hanno pressocchè sostituito le precedenti, oppure effettuando le riprese con webcam adattate allo scopo o con altri strumenti di ripresa di moderna concezione, per concludere con lo strumento principe per la fotografia astronomica e cioè la camera CCD, strumento idoneo per le riprese ad alta risoluzione e appositamente ideato per la ricerca scientifica di tutti i generi in astronomia. Ovviamente questi strumenti di ripresa devono essere collegati a telescopi astronomici dotati di montatura equatoriale motorizzata che deve essere ben stazionata al polo celeste, perchè possa ottimamente seguire la Luna nel suo moto nel cielo, ed è necessario inoltre inserire anche degli elementi ottici che possano aumentare la lunghezza focale dello strumento usato come le lenti di Barlow. Data la vicinanza del nostro satellite si può ottenere dei buoni risultati usando anche strumenti di piccole dimensioni.  </div></td></tr>
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</table>Antoniohttps://luna.uai.it/index.php?title=Alta_risoluzione&diff=275&oldid=prevAntonio il 18:35, 30 nov 20112011-11-30T18:35:55Z<p></p>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div>===== [[Image:Fig.3a mau.jpg|center|635x481px|Fig.3a mau.jpg]]<del class="diffchange diffchange-inline">&nbsp;&nbsp;&nbsp;</del>&nbsp; Fig.3 - Il polo Sud lunare, immagine di Maurizio e Francesca Cecchini (Montalcino, SI) i dati tecnici sono <del class="diffchange diffchange-inline">elencati </del>sopra<br> =====</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>===== [[Image:Fig.3a mau.jpg|center|635x481px|Fig.3a mau.jpg]]&nbsp; Fig.3 - Il polo Sud lunare, immagine di Maurizio e Francesca Cecchini (Montalcino, SI) i dati tecnici sono <ins class="diffchange diffchange-inline">specificati </ins>sopra<br> =====</div></td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div>===== [[Image:Fig.2a mau.jpg|center|650x488px|Fig.2a mau.jpg]]<del class="diffchange diffchange-inline">&nbsp;&nbsp;</del>&nbsp; Fig.2 - La zona del cratere Plato, immagine di Maurizio e Francesca Cecchini (Montalcino, SI) i dati sono <del class="diffchange diffchange-inline">elencati </del>sopra<br> =====</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>===== [[Image:Fig.2a mau.jpg|center|650x488px|Fig.2a mau.jpg]]&nbsp; Fig.2 - La zona del cratere Plato, immagine di Maurizio e Francesca Cecchini (Montalcino, SI) i dati sono <ins class="diffchange diffchange-inline">specificati </ins>sopra<br> =====</div></td></tr>
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</table>Antoniohttps://luna.uai.it/index.php?title=Alta_risoluzione&diff=273&oldid=prevAntonio il 17:28, 29 nov 20112011-11-29T17:28:08Z<p></p>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div>===== [[Image:Fig.4a ser.jpg|center|615x480px|Fig.4a ser.jpg]] <del class="diffchange diffchange-inline"> =====</del></div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>===== [[Image:Fig.4a ser.jpg|center|615x480px|Fig.4a ser.jpg]]Fig.4 - La Valle Alpina, immagine di Sergio Saltamonti (LI), telescopio OTA Meade 10", Barlow 2X, filtro IR, camera Skynix<br> =====</div></td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del class="diffchange diffchange-inline">===== </del>Fig.4 - La Valle Alpina, immagine di Sergio Saltamonti (LI), telescopio OTA Meade 10", Barlow 2X, filtro IR, camera Skynix<br> =====</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div></div></td></tr>
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</table>Antoniohttps://luna.uai.it/index.php?title=Alta_risoluzione&diff=272&oldid=prevAntonio il 17:24, 29 nov 20112011-11-29T17:24:32Z<p></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.5a cla.jpg|center|Fig.5a cla.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.5 - Mons e Gamma Piton, immagine di Claudio Vantaggiato (FG), elaborazione con Registax 5&nbsp;<br> =====</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.5a cla.jpg|center|Fig.5a cla.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.5 - Mons e Gamma Piton, immagine di Claudio Vantaggiato (FG), elaborazione con Registax 5&nbsp;<br> =====</div></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.3a mau.jpg|center|635x481px|Fig.3a mau.jpg]]&nbsp;&nbsp;&nbsp;&nbsp; Fig.3 - Il polo Sud lunare, immagine di Maurizio e Francesca Cecchini (Montalcino, SI) i dati tecnici sono elencati sopra<br> =====</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.3a mau.jpg|center|635x481px|Fig.3a mau.jpg]]&nbsp;&nbsp;&nbsp;&nbsp; Fig.3 - Il polo Sud lunare, immagine di Maurizio e Francesca Cecchini (Montalcino, SI) i dati tecnici sono elencati sopra<br> =====</div></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.1a mar.JPG|center|Fig.1a mar.JPG]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Fig.1 - Il cratere Copernico, immagine di Marco Vedovato (Predazzo, TN) i dati tecnici sono specificati sopra&nbsp;<br> =====</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.1a mar.JPG|center|Fig.1a mar.JPG]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Fig.1 - Il cratere Copernico, immagine di Marco Vedovato (Predazzo, TN) i dati tecnici sono specificati sopra&nbsp;<br> =====</div></td></tr>
</table>Antoniohttps://luna.uai.it/index.php?title=Alta_risoluzione&diff=271&oldid=prevAntonio il 17:19, 29 nov 20112011-11-29T17:19:30Z<p></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Questo settore del sito è dedicato alle immagini in alta risoluzione della Luna, che fanno parte di quelle riprese fotografiche effettuate a più alto ingrandimento dei dettagli della superficie lunare.<br>Il campo di lavoro degli osservatori lunari in questo contesto è vastissimo, avendo a disposizione esattamente la metà (e talvolta anche una quantità di superficie maggiore durante le condizioni favorevoli di librazione) della superficie totale lunare, ed inoltre in tutte le condizioni possibili di luce che si verificano durante il susseguirsi delle fasi lunari. Le tecniche di ripresa possono essere molteplici, partendo dalla tradizionale macchina fotografica a pellicola per i fotografi di tipo tradizionale (per la verità ormai molto rari), per poi passare alle moderne macchine digitali che ormai hanno pressocchè sostituito le precedenti, oppure effettuando le riprese con webcam adattate allo scopo o con altri strumenti di ripresa di moderna concezione, per concludere con lo strumento principe per la fotografia astronomica e cioè la camera CCD, strumento idoneo per le riprese ad alta risoluzione e appositamente ideato per la ricerca scientifica di tutti i generi in astronomia. Ovviamente questi strumenti di ripresa devono essere collegati a telescopi astronomici dotati di montatura equatoriale motorizzata che deve essere ben stazionata al polo celeste, perchè possa ottimamente seguire la Luna nel suo moto nel cielo, ed è necessario inoltre inserire anche degli elementi ottici che possano aumentare la lunghezza focale dello strumento usato come le lenti di Barlow. Data la vicinanza del nostro satellite si può ottenere dei buoni risultati usando anche strumenti di piccole dimensioni.  </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Questo settore del sito è dedicato alle immagini in alta risoluzione della Luna, che fanno parte di quelle riprese fotografiche effettuate a più alto ingrandimento dei dettagli della superficie lunare.<br>Il campo di lavoro degli osservatori lunari in questo contesto è vastissimo, avendo a disposizione esattamente la metà (e talvolta anche una quantità di superficie maggiore durante le condizioni favorevoli di librazione) della superficie totale lunare, ed inoltre in tutte le condizioni possibili di luce che si verificano durante il susseguirsi delle fasi lunari. Le tecniche di ripresa possono essere molteplici, partendo dalla tradizionale macchina fotografica a pellicola per i fotografi di tipo tradizionale (per la verità ormai molto rari), per poi passare alle moderne macchine digitali che ormai hanno pressocchè sostituito le precedenti, oppure effettuando le riprese con webcam adattate allo scopo o con altri strumenti di ripresa di moderna concezione, per concludere con lo strumento principe per la fotografia astronomica e cioè la camera CCD, strumento idoneo per le riprese ad alta risoluzione e appositamente ideato per la ricerca scientifica di tutti i generi in astronomia. Ovviamente questi strumenti di ripresa devono essere collegati a telescopi astronomici dotati di montatura equatoriale motorizzata che deve essere ben stazionata al polo celeste, perchè possa ottimamente seguire la Luna nel suo moto nel cielo, ed è necessario inoltre inserire anche degli elementi ottici che possano aumentare la lunghezza focale dello strumento usato come le lenti di Barlow. Data la vicinanza del nostro satellite si può ottenere dei buoni risultati usando anche strumenti di piccole dimensioni.  </div></td></tr>
<tr><td colspan="2" class="diff-lineno">Riga 70:</td>
<td colspan="2" class="diff-lineno">Riga 70:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.12a bru.jpg|center|640x480px|Fig.12a bru.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Fig.12 - Il cratere Moltke, immagine di Bruno Cantarella, telescopio con webcam ed elaborazione con Registax 6&nbsp;<br> =====</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.12a bru.jpg|center|640x480px|Fig.12a bru.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Fig.12 - Il cratere Moltke, immagine di Bruno Cantarella, telescopio con webcam ed elaborazione con Registax 6&nbsp;<br> =====</div></td></tr>
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<tr><td colspan="2" class="diff-lineno">Riga 92:</td>
<td colspan="2" class="diff-lineno">Riga 88:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.10a ant.jpg|center|592x501px|Fig.10a ant.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.10 - Il cratere Stadius, immagine di Antonio Marino, i dati tecnici sono specificati sopra<br> =====</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.10a ant.jpg|center|592x501px|Fig.10a ant.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.10 - Il cratere Stadius, immagine di Antonio Marino, i dati tecnici sono specificati sopra<br> =====</div></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.9a val.jpg|center|578x486px|Fig.9a val.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.9 - Il cratere Maurolycus, immagine di Valerio Fontani (FI), i dati tecnici sono specificati sopra<br> =====</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.9a val.jpg|center|578x486px|Fig.9a val.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.9 - Il cratere Maurolycus, immagine di Valerio Fontani (FI), i dati tecnici sono specificati sopra<br> =====</div></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.8a ser.jpg|center|631x469px|Fig.8a ser.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.8 - I crateri Theophilus, Cyrillus e Catharina, immagine di Sergio Saltamonti (LI)<br> =====</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.8a ser.jpg|center|631x469px|Fig.8a ser.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.8 - I crateri Theophilus, Cyrillus e Catharina, immagine di Sergio Saltamonti (LI)<br> =====</div></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.7a bru.jpg|center|Fig.7a bru.jpg]]&nbsp;&nbsp;&nbsp;&nbsp; Fig.7 - Il cratere Gutenberg, immagine di Bruno Cantarella (AL), telescopio MTO&nbsp;100/1000, Barlow 2X&nbsp;Apo con webcam<br> =====</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>===== [[Image:Fig.7a bru.jpg|center|Fig.7a bru.jpg]]&nbsp;&nbsp;&nbsp;&nbsp; Fig.7 - Il cratere Gutenberg, immagine di Bruno Cantarella (AL), telescopio MTO&nbsp;100/1000, Barlow 2X&nbsp;Apo con webcam<br> =====</div></td></tr>
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</table>Antoniohttps://luna.uai.it/index.php?title=Alta_risoluzione&diff=270&oldid=prevAntonio il 17:14, 29 nov 20112011-11-29T17:14:51Z<p></p>
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<td colspan='2' style="background-color: white; color:black;">← Versione meno recente</td>
<td colspan='2' style="background-color: white; color:black;">Versione delle 17:14, 29 nov 2011</td>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>'''<u>N.B. IL SITO SARA' UFFICIALMENTE ON-LINE IL 1 DICEMBRE PROSSIMO</u>'''  </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>'''<u>N.B. IL SITO SARA' UFFICIALMENTE ON-LINE IL 1 DICEMBRE PROSSIMO</u>'''  </div></td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del style="color: red; font-weight: bold; text-decoration: none;"><br>Questo settore del sito è dedicato alle immagini in alta risoluzione della Luna, che fanno parte di quelle riprese fotografiche effettuate a più alto ingrandimento dei dettagli della superficie lunare.<br>Il campo di lavoro degli osservatori lunari in questo contesto è vastissimo, avendo a disposizione esattamente la metà (e talvolta anche una quantità di superficie maggiore durante le condizioni favorevoli di librazione) della superficie totale lunare, ed inoltre in tutte le condizioni possibili di luce che si verificano durante il susseguirsi delle fasi lunari. Le tecniche di ripresa possono essere molteplici, partendo dalla tradizionale macchina fotografica a pellicola per i fotografi di tipo tradizionale (per la verità ormai molto rari), per poi passare alle moderne macchine digitali che ormai hanno pressocchè sostituito le precedenti, oppure effettuando le riprese con webcam adattate allo scopo o con altri strumenti di ripresa di moderna concezione, per concludere con lo strumento principe per la fotografia astronomica e cioè la camera CCD, strumento idoneo per le riprese ad alta risoluzione e appositamente ideato per la ricerca scientifica di tutti i generi in astronomia. Ovviamente questi strumenti di ripresa devono essere collegati a telescopi astronomici dotati di montatura equatoriale motorizzata che deve essere ben stazionata al polo celeste, perchè possa ottimamente seguire la Luna nel suo moto nel cielo, ed è necessario inoltre inserire anche degli elementi ottici che possano aumentare la lunghezza focale dello strumento usato come le lenti di Barlow. Data la vicinanza del nostro satellite si può ottenere dei buoni risultati usando anche strumenti di piccole dimensioni. </del></div></td><td colspan="2"> </td></tr>
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<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">Questo settore del sito è dedicato alle immagini in alta risoluzione della Luna, che fanno parte di quelle riprese fotografiche effettuate a più alto ingrandimento dei dettagli della superficie lunare.</ins><br><ins class="diffchange diffchange-inline">Il campo di lavoro degli osservatori lunari in questo contesto è vastissimo, avendo a disposizione esattamente la metà (e talvolta anche una quantità di superficie maggiore durante le condizioni favorevoli di librazione) della superficie totale lunare, ed inoltre in tutte le condizioni possibili di luce che si verificano durante il susseguirsi delle fasi lunari. Le tecniche di ripresa possono essere molteplici, partendo dalla tradizionale macchina fotografica a pellicola per i fotografi di tipo tradizionale (per la verità ormai molto rari), per poi passare alle moderne macchine digitali che ormai hanno pressocchè sostituito le precedenti, oppure effettuando le riprese con webcam adattate allo scopo o con altri strumenti di ripresa di moderna concezione, per concludere con lo strumento principe per la fotografia astronomica e cioè la camera CCD, strumento idoneo per le riprese ad alta risoluzione e appositamente ideato per la ricerca scientifica di tutti i generi in astronomia. Ovviamente questi strumenti di ripresa devono essere collegati a telescopi astronomici dotati di montatura equatoriale motorizzata che deve essere ben stazionata al polo celeste, perchè possa ottimamente seguire la Luna nel suo moto nel cielo, ed è necessario inoltre inserire anche degli elementi ottici che possano aumentare la lunghezza focale dello strumento usato come le lenti di Barlow. Data la vicinanza del nostro satellite si può ottenere dei buoni risultati usando anche strumenti di piccole dimensioni. </ins></div></td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[[Image:Fig.12a bru.jpg|center|640x480px|Fig.12a bru.jpg]]<br></div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">===== </ins>[[Image:Fig.12a bru.jpg|center|640x480px|Fig.12a bru.jpg]]<ins class="diffchange diffchange-inline">&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; Fig.12 - Il cratere Moltke, immagine di Bruno Cantarella, telescopio con webcam ed elaborazione con Registax 6&nbsp;<br> =====</ins></div></td></tr>
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</table>Antoniohttps://luna.uai.it/index.php?title=Alta_risoluzione&diff=268&oldid=prevAntonio il 20:36, 28 nov 20112011-11-28T20:36:52Z<p></p>
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<td colspan='2' style="background-color: white; color:black;">← Versione meno recente</td>
<td colspan='2' style="background-color: white; color:black;">Versione delle 20:36, 28 nov 2011</td>
</tr><tr><td colspan="2" class="diff-lineno">Riga 41:</td>
<td colspan="2" class="diff-lineno">Riga 41:</td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div><br></div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div><br></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[[Image:Fig.11a sep.jpg|center|746x417px|Fig.11a sep.jpg]]<br></div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">===== </ins>[[Image:Fig.11a sep.jpg|center|746x417px|Fig.11a sep.jpg]]<ins class="diffchange diffchange-inline">&nbsp;Fig.11 - Il cratere Copernico ripreso in diverse condizioni di luce, a sinistra da Sergio Saltamonti (LI) e Paolo Lazzarotti (MS)</ins><br> <ins class="diffchange diffchange-inline">=====</ins></div></td></tr>
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</table>Antoniohttps://luna.uai.it/index.php?title=Alta_risoluzione&diff=267&oldid=prevAntonio il 20:29, 28 nov 20112011-11-28T20:29:22Z<p></p>
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<td colspan='2' style="background-color: white; color:black;">← Versione meno recente</td>
<td colspan='2' style="background-color: white; color:black;">Versione delle 20:29, 28 nov 2011</td>
</tr><tr><td colspan="2" class="diff-lineno">Riga 51:</td>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div><br></div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div><br></div></td></tr>
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<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div>===== [[Image:Fig.10a ant.jpg|center|592x501px|Fig.10a ant.jpg]]<br> =====</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>===== [[Image:Fig.10a ant.jpg|center|592x501px|Fig.10a ant.jpg]]<ins class="diffchange diffchange-inline">&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.10 - Il cratere Stadius, immagine di Antonio Marino, i dati tecnici sono specificati sopra</ins><br> =====</div></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><br></div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div><ins class="diffchange diffchange-inline">===== [[Image:Fig.9a val.jpg|center|578x486px|Fig.9a val.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.9 - Il cratere Maurolycus, immagine di Valerio Fontani (FI), i dati tecnici sono specificati sopra</ins><br> <ins class="diffchange diffchange-inline">=====</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>−</td><td style="background: #ffa; color:black; font-size: smaller;"><div><del class="diffchange diffchange-inline">===== [[Image:Fig.9a val.jpg|center|578x486px|Fig.9a val.jpg]]&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;Fig.9 - Il cratere Maurolycus, immagine di Valerio Fontani (FI), i dati tecnici sono specificati sopra<br> =====</del></div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div> </div></td></tr>
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</table>Antonio