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Coronal Mass Ejections Observed at the Total Solar Eclipse on 13 November 2012
DOI: 10.1007/s11207-014-0476-z Bibcode: 2014SoPh..289.2587H

Hanaoka, Yoichiro; Nakazawa, Jun; Ohgoe, Osamu +2 more

White-light observations of the total solar eclipse on 13 November 2012 were made at two sites, where the totality occurred 35 min apart. The structure of the corona from the solar limb to a couple of solar radii was observed with a wide dynamic range and a high signal-to-noise ratio. An ongoing coronal mass ejection (CME) and a pre-CME loop struc…

2014 Solar Physics
PROBA-2 SOHO 13
A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. III. Catastrophe of the Eruptive Filament at a Magnetic Null Point and Formation of an Opposite-Handedness CME
DOI: 10.1007/s11207-014-0536-4 Bibcode: 2014SoPh..289.3747U

Grechnev, V. V.; Chertok, I. M.; Uralov, A. M. +4 more

Our analysis in Papers I and II (Grechnev et al., Solar Phys.289, 289, 2014b and Solar Phys.289, 1279, 2014c) of the 18 November 2003 solar event responsible for the 20 November geomagnetic superstorm has revealed a complex chain of eruptions. In particular, the eruptive filament encountered a topological discontinuity located near the solar disk …

2014 Solar Physics
SOHO 13
Analysis of Supergranule Sizes and Velocities Using Solar Dynamics Observatory (SDO)/ Helioseismic Magnetic Imager (HMI) and Solar and Heliospheric Observatory (SOHO)/ Michelson Doppler Imager (MDI) Dopplergrams
DOI: 10.1007/s11207-013-0330-8 Bibcode: 2014SoPh..289...11W

Williams, Peter E.; Pesnell, W. Dean; Beck, John G. +1 more

Co-temporal Doppler images from Solar and Heliospheric Observatory (SOHO)/Michelson Doppler Imager (MDI) and Solar Dynamics Observatory (SDO)/Helioseismic Magnetic Imager (HMI) have been analyzed to extract quantitative information about global properties of the spatial and temporal characteristics of solar supergranulation. Preliminary comparison…

2014 Solar Physics
SOHO 13
Modified Homogeneous Data Set of Coronal Intensities
DOI: 10.1007/s11207-014-0501-2 Bibcode: 2014SoPh..289.2697D

Minarovjech, M.; Rybanský, M.; Dorotovič, I. +1 more

The Astronomical Institute of the Slovak Academy of Sciences has published the intensities, recalibrated with respect to a common intensity scale, of the 530.3 nm (Fe XIV) green coronal line observed at ground-based stations up to the year 2008. The name of this publication is Homogeneous Data Set (HDS). We have developed a method that allows one …

2014 Solar Physics
SOHO 12
Fractal and Multifractal Properties of Active Regions as Flare Precursors: A Case Study Based on SOHO/MDI and SDO/HMI Observations
DOI: 10.1007/s11207-014-0500-3 Bibcode: 2014SoPh..289.2525E

Romano, P.; Zuccarello, F.; Ermolli, I. +3 more

Several studies indicate that fractal and multifractal parameters inferred from solar photospheric magnetic field measurements may help assessing the eruptive potential of Active Regions (ARs) and also predicting their flare activity. We further investigate this topic, by exploring the sensitivity of some parameters already used in the literature …

2014 Solar Physics
SOHO 12
Solar Wind Electron Strahls Associated with a High-Latitude CME: Ulysses Observations
DOI: 10.1007/s11207-014-0558-y Bibcode: 2014SoPh..289.4239L

Lazar, M.; Poedts, S.; Pomoell, J. +2 more

Counterstreaming beams of electrons are ubiquitous in coronal mass ejections (CMEs) - although their existence is not unanimously accepted as a necessary and/or sufficient signature of these events. We continue the investigation of a high-latitude CME registered by the Ulysses spacecraft on 18 - 19 January 2002 (Dumitrache, Popescu, and Oncica, So…

2014 Solar Physics
Ulysses 11
Automated Detection of Low-Contrast Solar Features Using the Phase-Congruency Algorithm
DOI: 10.1007/s11207-014-0538-2 Bibcode: 2014SoPh..289.3985F

Yang, Yunfei; Ji, Kaifan; Feng, Song +3 more

We propose a new feature-detection technique based on phase-congruency (PC) measurements to automatically recognize or enhance faint features in solar observations, such as off-limb coronal loops and umbral dots. Compared with other feature-detection methods that are based on gradient illuminance and imaging filtering, PC-based measurements are pa…

2014 Solar Physics
Hinode 11
May 2005 Halo CMEs and Galactic Cosmic Ray Flux Changes at Earth's Orbit
DOI: 10.1007/s11207-013-0439-9 Bibcode: 2014SoPh..289.1763A

Wawrzynczak, A.; Alania, M. V.; Ahluwalia, H. S. +2 more

The pressure corrected hourly data from the global network of cosmic ray detectors, measurements of the interplanetary magnetic field (IMF) intensity (B) at Earth's orbit and its components Bx, By, Bz (in the geocentric solar ecliptic coordinates) are used to conduct a comprehensive study of the galactic cosmic ray…

2014 Solar Physics
SOHO 10
Unusual Solar Radio Burst Observed at Decameter Wavelengths
DOI: 10.1007/s11207-013-0328-2 Bibcode: 2014SoPh..289..263M

Rucker, H. O.; Panchenko, M.; Konovalenko, A. A. +5 more

An unusual solar burst was observed simultaneously by two decameter radio telescopes UTR-2 (Kharkov, Ukraine) and URAN-2 (Poltava, Ukraine) on 3 June 2011 in the frequency range of 16 - 28 MHz. The observed radio burst had some unusual properties, which are not typical for the other types of solar radio bursts. Its frequency drift rate was positiv…

2014 Solar Physics
SOHO 9
Tracking Back the Solar Wind to Its Photospheric Footpoints from Wind Observations - A Statistical Study
DOI: 10.1007/s11207-014-0508-8 Bibcode: 2014SoPh..289.3109H

Li, Gang; Deng, Yuanyong; Tan, Baolin +2 more

It is of great importance to track the solar wind back to its photospheric source region and identify the related current sheets; this will provide key information for investigating the origin and predictions of the solar wind. We report a statistical study relating the photospheric footpoint motion and in-situ observation of current sheets in the…

2014 Solar Physics
SOHO 8