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Above the Noise: The Search for Periodicities in the Inner Heliosphere
DOI: 10.1007/s11207-017-1191-3 Bibcode: 2017SoPh..292..165T

De Moortel, Ineke; Threlfall, James; Conlon, Thomas

Remote sensing of coronal and heliospheric periodicities can provide vital insight into the local conditions and dynamics of the solar atmosphere. We seek to trace long (one hour or longer) periodic oscillatory signatures (previously identified above the limb in the corona by, e.g., Telloni et al. in Astrophys. J.767, 138, 2013) from their origin …

2017 Solar Physics
SOHO 10
Main Cause of the Poloidal Plasma Motion Inside a Magnetic Cloud Inferred from Multiple-Spacecraft Observations
DOI: 10.1007/s11207-017-1077-4 Bibcode: 2017SoPh..292...58Z

Wang, Yuming; Shen, Chenglong; Liu, Rui +3 more

Although the dynamical evolution of magnetic clouds (MCs) has been one of the foci of interplanetary physics for decades, only few studies focus on the internal properties of large-scale MCs. Recent work by Wang et al. (J. Geophys. Res.120, 1543, 2015) suggested the existence of the poloidal plasma motion in MCs. However, the main cause of this mo…

2017 Solar Physics
SOHO 9
An Early Diagnostics of the Geoeffectiveness of Solar Eruptions from Photospheric Magnetic Flux Observations: The Transition from SOHO to SDO
DOI: 10.1007/s11207-017-1081-8 Bibcode: 2017SoPh..292...62C

Grechnev, V. V.; Chertok, I. M.; Abunin, A. A.

In our previous articles (Chertok et al. in Solar Phys. 282, 175, 2013; Chertok et al. in Solar Phys. 290, 627, 2015), we presented a preliminary tool for the early diagnostics of the geoeffectiveness of solar eruptions based on the estimate of the total unsigned line-of-sight photospheric magnetic flux in accompanying extreme ultraviolet (EUV) ar…

2017 Solar Physics
SOHO 9
Detection of Coronal Mass Ejections Using Multiple Features and Space-Time Continuity
DOI: 10.1007/s11207-017-1107-2 Bibcode: 2017SoPh..292...91Z

Zhang, Ling; Yin, Jian-qin; Lin, Jia-ben +2 more

Coronal Mass Ejections (CMEs) release tremendous amounts of energy in the solar system, which has an impact on satellites, power facilities and wireless transmission. To effectively detect a CME in Large Angle Spectrometric Coronagraph (LASCO) C2 images, we propose a novel algorithm to locate the suspected CME regions, using the Extreme Learning M…

2017 Solar Physics
SOHO 9
Development and Parameters of a Non-Self-Similar CME Caused by the Eruption of a Quiescent Prominence
DOI: 10.1007/s11207-017-1167-3 Bibcode: 2017SoPh..292..143K

Grechnev, V. V.; Kuzmenko, I. V.

The eruption of a large quiescent prominence on 17 August 2013 and an associated coronal mass ejection (CME) were observed from different vantage points by the Solar Dynamics Observatory (SDO), the Solar-Terrestrial Relations Observatory (STEREO), and the Solar and Heliospheric Observatory (SOHO). Screening of the quiet Sun by the prominence produ…

2017 Solar Physics
SOHO 8
Anomalous Surge of the White-Light Corona at the Onset of the Declining Phase of Solar Cycle 24
DOI: 10.1007/s11207-017-1089-0 Bibcode: 2017SoPh..292...60L

Lamy, P.; Vibert, D.; Wojak, J. +1 more

In late 2014, when the current Solar Cycle 24 entered its declining phase, the white-light corona as observed by the LASCO-C2 coronagraph underwent an unexpected surge that increased its global radiance by 60%, reaching a peak value comparable to the peak values of the more active Solar Cycle 23. A comparison of the temporal variation of the white…

2017 Solar Physics
SOHO 8
Investigation of the Geoeffectiveness of Disk-Centre Full-Halo Coronal Mass Ejections
DOI: 10.1007/s11207-017-1102-7 Bibcode: 2017SoPh..292...79A

Valtonen, Eino; Ameri, Dheyaa

We studied the occurrence and characteristics of geomagnetic storms associated with disk-centre full-halo coronal mass ejections (DC-FH-CMEs). Such coronal mass ejections (CMEs) can be considered as the most plausible cause of geomagnetic storms. We selected front-side full-halo coronal mass ejections detected by the Large Angle and Spectrometric …

2017 Solar Physics
SOHO 8
SPIN: An Inversion Code for the Photospheric Spectral Line
DOI: 10.1007/s11207-017-1131-2 Bibcode: 2017SoPh..292..105Y

Mathew, Shibu K.; Yadav, Rahul; Tiwary, Alok Ranjan

Inversion codes are the most useful tools to infer the physical properties of the solar atmosphere from the interpretation of Stokes profiles. In this paper, we present the details of a new Stokes Profile INversion code (SPIN) developed specifically to invert the spectro-polarimetric data of the Multi-Application Solar Telescope (MAST) at Udaipur …

2017 Solar Physics
Hinode 8
Origin of Radio Enhancements in Type II Bursts in the Outer Corona
DOI: 10.1007/s11207-017-1148-6 Bibcode: 2017SoPh..292..127A

Valtonen, Eino; Pohjolainen, Silja; Al-Hamadani, Firas

We study interplanetary (IP) solar radio type II bursts from 2011 - 2014 in order to determine the cause of the intense enhancements in their radio emission. Type II bursts are known to be due to propagating shocks that are often associated with fast halo-type coronal mass ejections (CMEs). We analysed the radio spectral data and the white-light c…

2017 Solar Physics
SOHO 8
Initial In-flight Results: The Total Solar Irradiance Monitor on the FY-3C Satellite, an Instrument with a Pointing System
DOI: 10.1007/s11207-016-1027-6 Bibcode: 2017SoPh..292....9W

Wang, Hongrui; Li, Huiduan; Qi, Jin +1 more

The total solar irradiance (TSI) has been recorded daily since October 2013 by the Total Solar Irradiance Monitor (TSIM) onboard the FY-3C satellite, which is mainly designed for Earth observation. The TSIM has a pointing system to perform solar tracking using a sun sensor. The TSI is measured by two electrical substitution radiometers with tracea…

2017 Solar Physics
SOHO 7