J/A+A/383/719       Galilean Satellites mutual events 2002-2003    (Arlot, 2002)
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Predictions of the mutual events of the Galilean Satellites of Jupiter
occurring in 2002-2003
    Arlot J.-E.
   <Astron. Astrophys. 383, 719 (2002)>
   =2002A&A...383..719A
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ADC_Keywords: Planets ; Occultations ; Ephemerides
Keywords: planets and satellites: general -
          planets and satellites: individual: Jupiter

Abstract:
    Mutual occultations and eclipses of the Galilean satellites of Jupiter
    will occur in 2002-2003. This paper provides predictions of these
    events as well as information useful for their observations. Such
    events are uncommon, since they occur only every 6 years when the
    Earth and the Sun pass through the common orbital plane of the
    Galilean satellites. Therefore, we encourage professional and amateur
    astronomers to join the networks of observers in order to get as many
    observations as possible. Data on the predictions of the events are
    available on the web server of the Institut de Mecanique Celeste et
    de Calcul de Ephemerides (IMCCE) ( http://www.bdl.fr ).

File Summary:
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 FileName      Lrecl  Records   Explanations
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ReadMe            80        .   This file
events.dat       122      579   Predicted mutual events
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See also:
  http://www.bdl.fr/ephem/ephesat/phenjup2003_eng.html : Website
  J/A+A/314/312  : Galilean satellites mutual events in 1997 (Arlot 1996)
  J/A+AS/125/399 : Mutual phenomena of the Galilean satellites (Arlot+ 1997)

Byte-by-byte Description of file: events.dat
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   Bytes Format Units      Label   Explanations
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   1- 10  A10 "YYYY/MM/DD" Date    Date of the maximum of the event
  13- 19  A7    ---        Nature  Nature of the event (1)
      21  A1    ---        Type    [PAT] Type of eclipse (2)
  24- 25  I2    h          BP.h    ? UTC time of the beginning of the
                                      eclipse by the penumbra
  27- 28  I2    min        BP.m    ? UTC time of the beginning of the
                                      eclipse by the penumbra
  30- 32  F3.0  s          BP.s    ? UTC time of the beginning of the
                                      eclipse by the penumbra
  35- 36  I2    h          BS.h    ? TT time of the beginning of the eclipse by
                                   the shadow or beginning of the occultation
  38- 39  I2    min        BS.m    ? TT time of the beginning of the eclipse by
                                   the shadow or beginning of the occultation
  41- 43  F3.0  s          BS.s    ? TT time of the beginning of the eclipse by
                                   the shadow or beginning of the occultation
  46- 47  I2    h          BT.h    ? UTC time of the beginning of the totality
  49- 50  I2    min        BT.m    ? UTC time of the beginning of the totality
  52- 54  F3.0  s          BT.s    ? UTC time of the beginning of the totality
  57- 58  I2    h          Max.h   TT time of the maximum of the event
  60- 61  I2    min        Max.m   TT time of the maximum of the event
  63- 65  F3.0  s          Max.s   TT time of the maximum of the event
  68- 69  I2    h          ET.h    ? UTC time of the end of the totality
  71- 72  I2    min        ET.m    ? UTC time of the end of the totality
  74- 76  F3.0  s          ET.s    ? UTC time of the end of the totality
  79- 80  I2    h          ES.h    ? TT time of the end of the eclipse by the
                                     shadow or end of the occultation
  82- 83  I2    min        ES.m    ? TT time of the end of the eclipse by the
                                     shadow or end of the occultation
  85- 87  F3.0  s          ES.s    ? TT time of the end of the eclipse by the
                                     shadow or end of the occultation
  90- 91  I2    h          EP.h    ? TT time of the end of the
                                     eclipse by the penumbra
  93- 94  I2    min        EP.m    ? TT time of the end of the
                                     eclipse by the penumbra
  96- 98  F3.0  s          EP.s    ? TT time of the end of the
                                     eclipse by the penumbra
 101-105  F5.3  ---        Drop    [0,1]Flux drop (3)
 107-111  I5    s          Dur     ? Duration of the event (4)
 113-116  F4.1  ----       Dist    Apparent distance from the occulted or
                                   eclipsed satellite to the center of Jupiter
                                   in jovian radii
 118-122  F5.3  arcsec     Impact  Impact parameter
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Note (1): Nature of the event:
     1 OCC 2 means that satellite 1 occults satellite 2
     3 ECL 4 means that satellite 3 eclipses satellite 4
Note (2): Type of eclipse:
       P: partial
       A: annular
       T: total
   blank: eclipse by the penumbra
Note (3): Flux drop:
    if 0, grazing event with a very small signal to be detected;
    if 1, total event with a large signal easy to detect.
Note (4): No duration is indicated for grazing events.
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History: Copied at http://www.bdl.fr/ephem/ephesat/phenjup2003_eng.html
         J.E. Arlot, IMCCE/observatoire de Paris/CNRS-France
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(End)                                        Patricia Bauer [CDS]    15-Feb-2002
