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|a POSLANO DO SKCR
|b 2020-10-19
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|a BOD004
|b cze
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|a 521
|x Teoretická astronomie. Nebeská mechanika
|2 Konspekt
|9 6
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|a 521
|2 MRF
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080 |
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|a 520.8
|2 MRF
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1 |
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|a Orlando, Salvatore
|7 mub20191031909
|4 aut
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1 |
4 |
|a The sun as an X-ray star.
|n I.,
|p Deriving the emission measure distribution vs. temperature of the whole solar corona from the Yohkoh/SXT data /
|c S. Orlando, G. Peres and F. Reale.^^The sun as an X-ray star. II., Using the Yohkoh/SXT-derived solar emission measure vs. temperature to interpret stellar X-ray observation / G. Peres ... [et al.]
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|a Palermo :
|b Osservatorio Astronomico G.S. Vaiana,
|c 1999
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|a 46 s., [12] s. obr. příl. :
|b il.
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490 |
1 |
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|a Palermo astronomy preprints / Preprint ;
|v 5/99
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650 |
0 |
7 |
|a astrofyzika
|7 ph118641
|2 czenas
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0 |
7 |
|a astronomická pozorování
|7 ph118644
|2 czenas
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650 |
0 |
9 |
|a astronomical observations
|2 eczenas
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650 |
0 |
9 |
|a astrophysics
|2 eczenas
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700 |
1 |
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|a Peres, G.
|7 mub2015858801
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700 |
1 |
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|a Reale, F.
|7 mub2015858791
|4 aut
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710 |
2 |
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|a Palermo astronomy preprints
|4 pbl
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740 |
0 |
2 |
|a Sun as an X-ray star.
|n II.,
|p Using the Yohkoh/SXT-derived solar emission measure vs. temperature to interpret stellar X-ray observation
|
830 |
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0 |
|a Palermo astronomy preprints (Preprint) ;
|v 5/99
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