5918 Obs 20070415

From: ComHem (b.gimle@comhem.se)
Date: Mon Apr 16 2007 - 03:17:59 EDT

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    As implied by the field before the S(teady) and R(egular),
    the two middle #30587 obs are inaccurate appulses,
    and the third #29393 is a more accurate 90-deg 5% split of a 2 deg pair.
    Its period may mave been 15-20 sec?
    For #26934, I was quite uncertain about the star ID's
    when I wrote my notes (don't have my voice recorder at 5918)
    
    30587 07 005B   5918 G 20070415214133120 17 25 1931859+234684 68 S
    30587 07 005B   5918 G 20070415214144730 17 25 1944211+253636 19 S
    30587 07 005B   5918 G 20070415214159620 17 25 2000635+275550 19 S
    30587 07 005B   5918 G 20070415214221880 17 25 2027097+310813 78 S
    29393 06 037A   5918 G 20070415215751200 17 25 2022443+323858 78 R
    29393 06 037A   5918 G 20070415215808190 17 25 2046803+351386 88 R
    29393 06 037A   5918 G 20070415215839480 17 25 2134836+383715 28 R
    26934 01 044A   5918 G 20070415220831690 17 25 2048432+440046 39 S
    26934 01 044A   5918 G 20070415220901580 17 25 2212433+464800 39 S
    30588 07 005C   5918 G 20070415222403300 17 25 1925074+280446 48 S
    
    The observations above are, as I always do, reported in IOD format:
    http://www.satobs.org/position/IODformat.html
    
    -- Björn Gimle                                            --
    -- COSPAR 5918 WGS84,  +18.10127 (E), +59.29813 (N), 44 m --
    -- COSPAR 5919, MALMA, +18.6206  (E), +59.2615  (N), 33 m --
    -- COSPAR 5920, FRUVIK,+18.4820  (E), +59.3260  (N), 11 m --
    
    
    
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