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Solar Irradiance Variations: From Current Measurements to Long-Term Estimates
DOI: 10.1007/s11207-005-6499-8 Bibcode: 2004SoPh..224..197S

Solanki, Sami K.; Krivova, Natalie A.

Variations of solar total and spectral irradiance are prime solar quantities purported to have an influence on the Earth's climate. Quantitative estimates of irradiance over as long a time as possible are needed to judge their effectiveness in forcing the climate. In order to do this reliably, first the measured record must be reproduced and a fee…

2004 Solar Physics
SOHO 46
Geoeffectiveness of interplanetary shocks during solar minimum (1995 1996) and solar maximum (2000)
DOI: 10.1023/B:SOLA.0000035045.65224.f3 Bibcode: 2004SoPh..221..361E

Echer, E.; Gonzalez, W. D.; Alves, M. V.

Plasma and magnetic field parameter variations across fast forward interplanetary shocks are analyzed during the last solar cycle minimum (1995-1996, 15 shocks), and maximum year 2000 (50 shocks). It was observed that the solar wind velocity and magnetic field strength variation across the shocks were the parameters better correlated with Dst. Sup…

2004 Solar Physics
SOHO 42
Separators in 3D Quiet-Sun Magnetic Fields
DOI: 10.1007/s11207-004-3259-0 Bibcode: 2004SoPh..225...21C

Priest, E. R.; Parnell, C. E.; Close, R. M.

At the confluence of four regions of different magnetic connectivity lies a distinct topological candidate for coronal heating, namely the magnetic separator. In this study, a method for tracing separator curves is developed and the statistical properties of separators in coronal fields are subsequently explored by analysing a model field with an …

2004 Solar Physics
SOHO 41
Correction of Offset in MDI/SOHO Magnetograms
DOI: 10.1023/B:SOLA.0000021822.07430.d6 Bibcode: 2004SoPh..219...39L

Liu, Yang; Hoeksema, J. Todd; Zhao, Xuepu

Shutter noise induces a small random shift of the zero point in full-disk magnetograms obtained by the Michelson Doppler Imager (MDI) instrument aboard SOHO. In this paper, we develop a method to remove this offset by fitting the distribution of the magnetic field strength with a Gaussian function (Ulrich et al., 2002). We also discover a systemat…

2004 Solar Physics
SOHO 40
Prominence corona transition region plasma diagnostics from SOHO observations
DOI: 10.1007/s11207-004-5101-0 Bibcode: 2004SoPh..223...95C

Vial, J. -C.; Rovira, M.; Cirigliano, D.

New results concerning prominence observations and in particular the prominence-corona transition region (PCTR) are presented. In order to cover a temperature range from 2 × 104 to 7 × 105 K, several emission lines in many different ionization states were observed with SUMER and CDS on board SOHO. EM and DEM were measured thr…

2004 Solar Physics
SOHO 39
On Re-sampling of Solar Images
DOI: 10.1023/B:SOLA.0000021743.24248.b0 Bibcode: 2004SoPh..219....3D

DeForest, C. E.

Digital image data are now commonly used throughout the field of solar physics. Many steps of image data analysis, including image co-alignment, perspective reprojection of the solar surface, and compensation for solar rotation, require re-sampling original telescope image data under a distorting coordinate transformation. The most common image re…

2004 Solar Physics
SOHO 38
On the Coronal Mass Ejection onset and Coronal Dimming
DOI: 10.1023/B:SOLA.0000022946.98359.63 Bibcode: 2004SoPh..219..315H

Howard, Timothy A.; Harrison, Richard A.

A comprehensive case and statistical study of CME onsets has been conducted on the solar limb using the CDS, LASCO and EIT instruments aboard the SOHO spacecraft. This is the first dedicated campaign to establish firmly the EUV signatures of CME onsets and is based on a series of low-corona observing campaigns made in 2002. The event database cons…

2004 Solar Physics
SOHO 33
A High-Speed Erupting-Prominence CME: A Bridge Between Types
DOI: 10.1023/B:SOLA.0000022996.53206.9d Bibcode: 2004SoPh..219..301F

Feynman, Joan; Ruzmaikin, Alexander

Several studies have indicated that there may be two distinct types of coronal mass ejections (CMEs); a high-velocity bright energetic type associated with flares, and a smaller slower less impressive type associated with erupting prominences. How valid is this distinction? We analyze a CME combining attributes of both types, a high-velocity brigh…

2004 Solar Physics
SOHO 33
Structure Properties of Supergranulation and Granulation
DOI: 10.1023/B:SOLA.0000033368.00217.de Bibcode: 2004SoPh..221...33B

Kosovichev, A. G.; Pietropaolo, E.; Duvall, T. L., Jr. +3 more

We investigate spatial dislocation ordering of the solar structures associated with supergranulation and granulation scales. The supergranular and granular structures are automatically segmented from time-distance divergence maps and from broad-band images, respectively. The spatial dislocation ordering analysis is accomplished by applying the sta…

2004 Solar Physics
SOHO 32
Oscillations in the Umbral Atmosphere
DOI: 10.1023/B:SOLA.0000035065.10112.fc Bibcode: 2004SoPh..221..237B

Foley, C. R.; Fredvik, T.; Kjeldseth-Moe, O. +2 more

The results of simultaneous observations of oscillations in the chromosphere, transition region, and corona above nine sunspots are presented. The data are obtained through coordinated observing with the Solar and Heliospheric Observatory — SOHO and the Transition Region And Coronal Explorer — TRACE. Oscillations are detected above each umbra. The…

2004 Solar Physics
SOHO 30