The Middle Atmospheric Ozone Response to the 11-Year Solar Cycle

2007 ◽  
pp. 273-286 ◽  
Author(s):  
Y. Calisesi ◽  
K. Matthes
Keyword(s):  
Solar Cycle ◽  
Atmospheric Ozone

The Middle Atmospheric Ozone Response to the 11-Year Solar Cycle

2007 ◽  
Vol 125 (1-4) ◽  
pp. 273-286 ◽  
Author(s):  
Y. Calisesi ◽  
K. Matthes
Keyword(s):  
Solar Cycle ◽  
Atmospheric Ozone

scholarly journals Possible variations in atmospheric ozone related to the eleven-year solar cycle

1978 ◽  
Vol 5 (10) ◽  
pp. 817-820 ◽  
Author(s):  
Joyce E. Penner ◽  
Julius S. Chang
Keyword(s):  
Solar Cycle ◽  
Atmospheric Ozone

Calculated Coronal Magnetic Fields and Their Comparison with the Coronal Structures as Observed during Five Solar Eclipses

1994 ◽  
Vol 144 ◽  
pp. 559-564
Author(s):  
P. Ambrož ◽  
J. Sýkora
Keyword(s):  
Magnetic Field ◽  
Solar Cycle ◽  
Magnetic Fields ◽  
Solar Corona ◽  
Coronal Magnetic Field ◽  
Coronal Magnetic Fields ◽  
Solar Eclipses ◽  
Coronal Structures

AbstractWe were successful in observing the solar corona during five solar eclipses (1973-1991). For the eclipse days the coronal magnetic field was calculated by extrapolation from the photosphere. Comparison of the observed and calculated coronal structures is carried out and some peculiarities of this comparison, related to the different phases of the solar cycle, are presented.

The Hemispheric Sign Rule of Current Helicity during the Rising Phase of Cycle 23

2000 ◽  
Vol 179 ◽  
pp. 303-306
Author(s):  
S. D. Bao ◽  
G. X. Ai ◽  
H. Q. Zhang
Keyword(s):  
Solar Cycle ◽  
Southern Hemisphere ◽  
Northern Hemisphere ◽  
Active Regions ◽  
Hemispheric Preference ◽  
Current Helicity

AbstractWe compute the signs of two different current helicity parameters (i.e., αbestandHc) for 87 active regions during the rise of cycle 23. The results indicate that 59% of the active regions in the northern hemisphere have negative αbestand 65% in the southern hemisphere have positive. This is consistent with that of the cycle 22. However, the helicity parameterHcshows a weaker opposite hemispheric preference in the new solar cycle. Possible reasons are discussed.

Prominences and Solar Activity

1979 ◽  
Vol 44 ◽  
pp. 357-372
Author(s):  
Z. Švestka
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
List Type ◽  
Type Number ◽  
Flare Loops ◽  
Filament Activation

The following subjects were discussed:(1)Filament activation(2)Post-flare loops.(3)Surges and sprays.(4)Coronal transients.(5)Disk vs. limb observations.(6)Solar cycle variations of prominence occurrence.(7)Active prominences patrol service.Of all these items, (1) and (2) were discussed in most detail and we also pay most attention to them in this report. Items (3) and (4) did not bring anything new when compared with the earlier invited presentations given by RUST and ZIRIN and therefore, we omit them.

ROTATIONAL SPECTROSCOPY OF NEWLY DETECTED ATMOSPHERIC OZONE DEPLETERS: CF3CH2Cl, CF3CCl3, AND CF2ClCCl3

2015 ◽  
Author(s):  
Zbigniew Kisiel ◽  
Emilio Cocinero ◽  
Francisco Basterretxea ◽  
Patricia Ecija ◽  
Iciar Uriarte ◽  
...  
Keyword(s):  
Rotational Spectroscopy ◽  
Atmospheric Ozone
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