linkages between the atmosphere on the Earth and sun Phần 2 ppsx
linkages between the atmosphere on the Earth and sun Phần 2 ppsx
... smaller and smaller the deeper in the star
one’s inferences are drawn.
Fig. 12 Doppler images of the Sun obtained by the solar oscillations investigation using the
Michelson Doppler imager on the ... missing is the almost horizontal passage through the very
thin annulus occupying the space between its deepest penetration level and that of
the second wave: the...
linkages between the atmosphere on the Earth and sun Phần 6 ppsx
... from the latter
Waves in Polar Coronal Holes 28 3
2 Observation and Results
We observed the North polar coronal hole with EIS onboard Hinode, on and off the
limb with the 2
00
slit on 10 October 20 07. ... nonthermal motions. The expression
for the FWHM is
FWHM D
"
W
2
inst
C 4 ln 2
Â
c
Ã
2
Â
2k T
i
M
i
C
2
Ã
#
1 =2
; (1)
where T
i
, M
i
,and are,...
linkages between the atmosphere on the Earth and sun Phần 1 docx
... light on the constitution of
the Sun. In 1885, the Royal Society, London, constituted the Indian Observatories
Committee comprised of the Astronomer Royal, and a few Fellows of the Royal and
Royal ... showed
the CN bands and the C2 Swan bands in the head, while the tail showed bands due
to CO. He was ably assisted in the observations by his wife Mary.
Contents i...
linkages between the atmosphere on the Earth and sun Phần 3 pps
... sign, depending
on the sense of rotation (orientation of the field vector). The magnitudes of these
two effects depend on the competition between the Larmor precession rate and the
damping rate, ... performed
Chromospheric and Coronal Polarization Diagnostics 121
Q
I
3
8
p
2
h
.1
2
/.3 cos
2
Â
B
1/ C .1C
2
/.cos
2
Â
B
1/
i
.3 cos
2
Â
B
1/ F;
(3)
U...
linkages between the atmosphere on the Earth and sun Phần 4 potx
... in the upper layers of the photosphere and the chromosphere
and consequently no substantial coupling between waves and the magnetic field
would occur in these layers. On the other hand, if there ... valid on scales smaller than 0.3
00
. In fact,
simulations suggest constant angular distribution within ˙50
ı
from the horizon-
tal direction on a scale of 0:05
00
. On...
linkages between the atmosphere on the Earth and sun Phần 5 doc
... v
z
(left)
and horizontal velocity v
x
(right), where the x-axisisparalleltothebottom of the panels
26 2 C.E. Parnell and A.L. Haynes
key role in linking the magnetic fields from the Sun and Earth and ... Weiss (20 08) and the reviews
by Solanki (20 03) and Thomas and Weiss (20 04).
2 Umbral Magnetoconvection
In a broad sense, there are two competing models of t...
linkages between the atmosphere on the Earth and sun Phần 7 pps
... fields (and how they
can be measured), then sunspots themselves as well as the quiet Sun, before mov-
ing upwards into the atmosphere and the corona, with the violence of coronal mass
ejections and ... 3:9 1 Ä Ä 3:9
The Solar-Stellar Connection 337
4 The Ca II H & K Sun
The variation of the solar emission in the cores of the calcium resonance lines and
t...
linkages between the atmosphere on the Earth and sun Phần 8 pps
... with the first point 1 year after the sunspot minimum. We find strong
correlation between the rates of rise and the amplitudes of the sunspot cycles.
1 .2 1.4 1.6 1.8 2 2 .2 2.4
50
100
150
20 0
Rise ... 0.50 and 90:16% for sunspot numbers;
(2) 0. 42 and 82: 12% for group sunspots; (3) 0.31 and 67:3% for sunspot areas;
and (4) 0.33 and 41%for10:7 cm radio flux....
linkages between the atmosphere on the Earth and sun Phần 9 potx
... phase of the second flare and its evolution in correlation with ribbon
separation provide evidence for the cause of the CME eruption. The propagation and
orientation of the CME with respect to the ... case, and through (2) , the conductive cooling time t
c
,whichwas
77 s for this flare. The five flares yielded t
c0
values between 1,088 and 2, 016 s and t
c
values bet...
linkages between the atmosphere on the Earth and sun Phần 10 potx
... correlation between the polar field at the
minimum and the strength of the next sunspot cycle when the turbulent diffusiv-
ity inside the convection zone is sufficiently high [Jiang et al. 20 07, MNRAS, ... 1 ,20 7 s for the thermal mode and 26 s
for the slow mode, and damping per wave period of 0.06 for the thermal mode and
7.64 for the slow mode. The thermal...