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J/A+AS/110/351 Sun observations in 1992 (Sanchez+, 1995)
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L'astrolabe du ROA. Observations du Soleil en 1992. Observations of the Sun at
ROA astrolabe in 1992.
Sanchez M., Parra F., Soler M., Soto R.
<Astron. Astrophys. Suppl. Ser. 110, 351 (1995)>
=1995A&AS..110..351S (SIMBAD/NED Reference)
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ADC_Keywords: Sun; Astrometric data
Keywords: astrometry - Sun: general; fundamental parameters
Description:
The results of an observational campaign of the Sun are reported.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1 24 28 UT0-UTC and Delta{phi} values following IERS
(International Earth Rotation System)
table2 83 59 Results for 1992 solar campaign at 60deg height
table1.tex 150 32 LaTeX version of table1
table2.tex 318 77 LaTeX version of table2
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Byte-by-byte Description of file: table1
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Bytes Format Units Label Explanations
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1- 5 I5 d MJD Modified Julian day
11- 14 F4.2 arcsec Dphi Variation of local latitude
18- 23 F6.3 s UT0-UTC UT0-UTC value
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Byte-by-byte Description of file: table2
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Bytes Format Units Label Explanations
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2- 5 I4 --- Date Date (Month, day)
7- 13 F7.1 d MJD Modified Julian day
16- 17 I2 --- Obs Observers (1)
19- 24 F6.3 arcsec BSE []? East upper limb passage observation residual
25 A1 --- n_BSE [*] Note on BSE (2)
26- 31 F6.3 arcsec BIE []? East lower limb passage observation residual
32 A1 --- n_BIE [*] Note on BIE (2)
33- 38 F6.3 arcsec BIW []? West lower limb passage observation residual
39 A1 --- n_BIW [*] Note on BIW (2)
40- 45 F6.3 arcsec BSW []? West upper limb passage observation residual
46 A1 --- n_BSW [*] Note on BSW (2)
47- 52 F6.3 s dRA []? Offset in right ascension
55- 59 F5.3 s e_dRA []? rms uncertainty on dRA
61- 65 F5.2 arcsec Y []? Y=Delta(z) +Delta(delta)cos(S) (3)
67- 71 F5.2 arcsec DS []? Correction in calculated apparent
demi-diameter
73- 76 F4.2 arcsec e_DS []? rms uncertainty on DS
78- 83 F6.2 arcsec S []? Semi-diameter rapported to the
astronomical unit
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Note (1): Observators: 6: M. Sanchez; 7: F. Parra; 13: R. Soto; 16: M. Soler
Note (2): A '*' signifies that the limbs are not observed (clouds, errors, etc.)
Note (3): Y=Delta(z) + Delta(delta)cos(S) where,
Delta(z) is the correction in zenithal distance, Delta(delta) is the
correction in declination and S is the angle at the celestial object
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(End) Patricia Bauer [CDS] 13-Dec-1994