dc.contributor.author |
Kameswara Rao, N |
|
dc.date.accessioned |
2021-02-14T06:01:21Z |
|
dc.date.available |
2021-02-14T06:01:21Z |
|
dc.date.issued |
1995 |
|
dc.identifier.citation |
Sinha,B and Bhattacharya, M eds, From Astronomy to Astrophysics:Proceedings of symposium on Astronomy and Astrophysics, pp. 149 - 170 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2248/7622 |
|
dc.description |
© Saha Institute of Nuclear Physics |
en_US |
dc.description.abstract |
"The
abrupt
termination
of
solar
and
stellar
spectrum
below
A 2900
has
been
a
great
handicap
to
the
advancement
of
our
knowledge
of
the
heavenly
bodies
; because
the
information
gained
from
the
study
of
the
spectrum
beyond
A,
2900
is
not
sufficient
'to
explain
the
problems
of
stellar
mechanisms
operative
there." |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Saha Institute of Nuclear Physics |
en_US |
dc.subject |
UV Astronomy |
en_US |
dc.subject |
Solar UV Spectrum |
en_US |
dc.subject |
Chromospheric & Coronal Studies |
en_US |
dc.title |
UV astronomy and stellar chromosphere |
en_US |
dc.type |
Book chapter |
en_US |