Search Publications

The Automatic Predictability of Super Geomagnetic Storms from halo CMEs associated with Large Solar Flares
DOI: 10.1007/s11207-006-0164-8 Bibcode: 2006SoPh..238..141S

Yang, Guo; Wang, Haimin; Yurchyshyn, Vasyl +3 more

We investigate the relationship between magnetic structures of coronal mass ejection (CME) source regions and geomagnetic storms, in particular, the super storms when the Dst index decreases below −200 nT. By examining all full halo CMEs that erupted between 1996 and 2004, we selected 73 events associated with M-class and X-class solar …

2006 Solar Physics
SOHO 23
Multiple Triangulation Analysis: another approach to determine the orientation of magnetic flux ropes
DOI: 10.5194/angeo-24-1759-2006 Bibcode: 2006AnGeo..24.1759Z

Wei, Y.; Zong, Q. -G.; Dunlop, M. W. +5 more

Another approach (Multiple Triangulation Analysis, MTA) is presented to determine the orientation of magnetic flux rope, based on 4-point measurements. A 2-D flux rope model is used to examine the accuracy of the MTA technique in a theoretical way. It is found that the precision of the estimated orientation is dependent on both the spacecraft sepa…

2006 Annales Geophysicae
Cluster 23
The Prediction of a Supersoft X-Ray Phase during the 2006 Outburst of RS Ophiuchi
DOI: 10.1086/504427 Bibcode: 2006ApJ...642L..53H

Kato, Mariko; Hachisu, Izumi

RS Ophiuchi is one of the well-observed recurrent novae and also a candidate progenitor of Type Ia supernovae. Its sixth recorded outburst was discovered on 2006 February 12. Detection of a supersoft X-ray phase will provide us with a firm confirmation of hydrogen shell burning on the white dwarf, and its turn-on/turnoff dates strongly constrain t…

2006 The Astrophysical Journal
XMM-Newton 23
Multi-Site Spectrographic and Heliographic Observations of Radio Fine Structure on April 10, 2001
DOI: 10.1007/s11207-006-0111-8 Bibcode: 2006SoPh..237..397C

Tan, Chengming; Yan, Yihua; Huang, Guangli +5 more

We present results of the first simultaneous observations of zebra patterns (ZPs) with super-fine spiky structure in the microwave range made at two observatories ∼1000 km apart (Beijing and Nanjing, China). The fine structure was recorded by a spectra polarimeter in the 5.2 - 7.6 and 2.8 - 3.6 GHz ranges at the Huairou station and by the spectrom…

2006 Solar Physics
SOHO 23
Light dark matter annihilations into two photons
DOI: 10.1016/j.physletb.2006.08.036 Bibcode: 2006PhLB..641..247B

Boehm, C.; Orloff, J.; Salati, P.

We compute the pair annihilation cross section of light (spin-0) dark matter particles into two photons and discuss the detectability of the monochromatic line associated with these annihilations.

2006 Physics Letters B
INTEGRAL 22
Star formation in QSO host galaxies
DOI: 10.1016/j.newar.2006.06.019 Bibcode: 2006NewAR..50..650C

Lacy, Mark; Stockton, Alan; Canalizo, Gabriela +1 more

Many of the conditions that are necessary for starbursts appear to be important in the triggering of QSOs. However, it is still debatable whether starbursts are ubiquitously present in galaxies harboring QSOs. In this paper we review our current knowledge from observations of the role of starbursts in different types of QSOs. Post-starburst stella…

2006 New Astronomy Reviews
eHST 22
Sensitivity of solar off-limb line profiles to electron density stratification and the velocity distribution anisotropy
DOI: 10.1051/0004-6361:20042568 Bibcode: 2006A&A...445..735R

Solanki, S. K.; Raouafi, N. -E.

The effect of the electron density stratification on the intensity profiles of the H I Ly-α line and the O VI and Mg X doublets formed in solar coronal holes is investigated. We employ an analytical 2-D model of the large scale coronal magnetic field that provides a good representation of the corona at the minimum of solar activity. We use the mas…

2006 Astronomy and Astrophysics
SOHO 22
Spectral line width decrease in the solar corona: resonant energy conversion from Alfvén to acoustic waves
DOI: 10.1051/0004-6361:20065805 Bibcode: 2006A&A...456L..13Z

Oliver, R.; Zaqarashvili, T. V.; Ballester, J. L.

Context: .Observations reveal an increase with height of the line width of several coronal spectral lines probably caused by outwardly propagating Alfvén waves. However, the spectral line width sometimes shows a sudden decrease at a height ~0.1-0.2 R, where the ratio of sound to Alfvén speeds may approach unity.
Aims: .To explain t…

2006 Astronomy and Astrophysics
SOHO 22
To the depths of Venus: Exploring the deep atmosphere and surface of our sister world with Venus Express
DOI: 10.1016/j.pss.2006.04.034 Bibcode: 2006P&SS...54.1263B

Drossart, Pierre; Baines, Kevin H.; Piccioni, Giuseppe +6 more

With its comprehensive suite of near-infrared instruments, Venus Express will perform the first detailed global exploration of the depths of the thick Venusian atmosphere. Through the near-daily acquisition of Visible and Infrared maps and spectra, three infrared-sensing instruments - the Planetary Fourier Spectrometer (PFS), the Venus Monitoring …

2006 Planetary and Space Science
VenusExpress 22
Evolution of Electric Currents Associated with Two M-Class Flares
DOI: 10.1007/s11207-006-0120-7 Bibcode: 2006SoPh..239..137T

Tan, Baolin; Ji, Haisheng; Huang, Guangli +3 more

Using one-minute cadence vector magnetograms from Big Bear Solar Observatory (BBSO), we analyze the temporal behavior of derived longitudinal electric currents associated with two flares on July 26, 2002. One of the events is an M1.0 flare which occurred in active region NOAA 10044, while the other is an M8.7 flare in the adjacent region 10039. Ra…

2006 Solar Physics
SOHO 22