Спостереження Сонячного затемнення 22 липня 1990 року

Scientists of Astronomic Observatory at the Lviv Ivan Franko National
 University observed a full solar eclipse on July 22nd 1990 at the most conve
 
 nient place village Marcovo of Anadyr district of Magadan region ( Russian
 Federation).
 The place h...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Праці наукового товариства ім. Шевченка
Datum:2011
ISSN:1563-3569
Hauptverfasser: Благодир, Я., Ковальчук, М., Гірняк, М., Лаба, І.
Format: Artikel
Sprache:Ukrainisch
Veröffentlicht: Західний науковий центр НАН України і МОН України 2011
Schlagworte:
Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/75114
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren:Спостереження Сонячного затемнення 22 липня 1990 року / Я. Благодир, М. Ковальчук, М. Гірняк, І. Лаба // Праці Наукового товариства ім. Шевченка. — Л., 2011. — Т. 8: Фізичний збірник. — С. 44-54. — Бібліогр.: 6 назв. — укр.

Institution

Digital Library of Periodicals of National Academy of Sciences of Ukraine
Beschreibung
Zusammenfassung:Scientists of Astronomic Observatory at the Lviv Ivan Franko National
 University observed a full solar eclipse on July 22nd 1990 at the most conve
 
 nient place village Marcovo of Anadyr district of Magadan region ( Russian
 Federation).
 The place has been chosen due to the maximal altitude of the
 Sun above the horizon -40°
 The three-objective coronograph was constructed for observations There
 were obtained 33 photographs of the inner and middle corona The corona
 was photographed in integral light in blue and yellow ranges of the spectrum
 and in polarized light 
 The solar corona on July 22 nd 1990 is of the shape that corresponds to
 corona of the maximum of solar activity The distribution of brightness in the
 corona does not depend on heliographic latitude The compression of corona
 reaches its maximum value at far (>1.5) distances from the Sun The colour
 temperature was determined at the middle distance of 1.5 - it turned out to
 be 5160 K The value and plane of polarization were calculated the radiation
 of corona has got a radial polarization
ISSN:1563-3569