Article
Astronomy & Astrophysics
B. Ramsey, E. Verwichte, H. Morgan
Summary: This study presents a wavelet-based method that automatically detects and tracks the intensity evolution of bright points (BPs) in the solar corona. The results show significant periodicity and power-law relationships between the BP lifetime and maximum diameter. The findings provide insights into the underlying physical mechanisms.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
D. J. Pascoe, I De Moortel, P. Pagano, T. A. Howson
Summary: This study considers the behavior of Alfven waves propagating in a medium with random density perturbations. The interaction between the Alfven waves and the medium generates reflections most efficiently when their wavelength is comparable to the spatial scale of the density perturbations. This leads to the generation of quasi-periodic oscillations, and the periods of oscillation are no longer solely associated with the driver. Multiple wave reflections cause oscillatory power to be retained at low altitudes, increasing opportunities for heating at those locations.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Nancy Narang, Kalugodu Chandrashekhar, Shahin Jafarzadeh, Bernhard Fleck, Mikolaj Szydlarski, Sven Wedemeyer
Summary: This study presents a statistical analysis of oscillation power distribution in a plage region in an active region using observations from ALMA, IRIS, and SDO. The results show that there is no significant association between ALMA oscillations and IRIS/AIA oscillations. It is speculated that the non-association is due to variations in the height of formation of the millimeter continuum observed by ALMA and the different nature of ALMA oscillations compared to IRIS and AIA oscillations.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
V Andretta, A. Bemporad, Y. De Leo, G. Jerse, F. Landini, M. Mierla, G. Naletto, M. Romoli, C. Sasso, A. Slemer, D. Spadaro, R. Susino, D-C Talpeanu, D. Telloni, L. Teriaca, M. Uslenghi, E. Antonucci, F. Auchere, D. Berghmans, A. Berlicki, G. Capobianco, G. E. Capuano, C. Casini, M. Casti, P. Chioetto, V Da Deppo, M. Fabi, S. Fineschi, F. Frassati, F. Frassetto, S. Giordano, C. Grimani, P. Heinzel, A. Liberatore, E. Magli, G. Massone, M. Messerotti, D. Moses, G. Nicolini, M. Pancrazzi, M-G Pelizzo, P. Romano, U. Schuehle, M. Stangalini, Th Straus, C. A. Volpicelli, L. Zangrilli, P. Zuppella, L. Abbo, R. Aznar Cuadrado, R. Bruno, A. Ciaravella, R. D'Amicis, P. Lamy, A. Lanzafame, A. M. Malvezzi, P. Nicolosi, G. Nistico, H. Peter, C. Plainaki, L. Poletto, F. Reale, S. K. Solanki, L. Strachan, G. Tondello, K. Tsinganos, M. Velli, R. Ventura, J-C Vial, J. Woch, G. Zimbardo
Summary: Observations by Metis of a CME reveal that most features seen in visible-light images are also visible in Ly-alpha images, although the latter appear more structured. The estimated expansion velocity of the event is below 140 km/s, suggesting Doppler dimming effects do not significantly reduce Ly-alpha emission from the CME.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
A. Bemporad, V Andretta, R. Susino, S. Mancuso, D. Spadaro, M. Mierla, D. Berghmans, E. D'Huys, A. N. Zhukov, D-C Talpeanu, R. Colaninno, P. Hess, J. Koza, S. Jejcic, P. Heinzel, E. Antonucci, V Da Deppo, S. Fineschi, F. Frassati, G. Jerse, F. Landini, G. Naletto, G. Nicolini, M. Pancrazzi, M. Romoli, C. Sasso, A. Slemer, M. Stangalini, L. Teriaca
Summary: This study combines data acquired by remote-sensing instruments on board Solar Orbiter to investigate the eruptions and different source regions. By using different 3D reconstruction methods, the expansion process of the eruptions from their source region to the intermediate corona is traced. The analysis of Metis data provides new insights into solar eruptions, including the formation of a post-CME current sheet and the measurement of plasma temperature gradient. The application of the polarization ratio technique improves the accuracy of the data and constrains the 3D plasma distribution.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
S. L. Yardley, D. H. Brooks, D. Baker
Summary: The study revealed the presence of upflows at both eastern and western boundaries of all active regions, with every line profile showing a blue wing asymmetry. In most cases, the intensity ratio of the minor high-speed asymmetric Gaussian component compared to the main component is relatively small, but in a minority of cases, the ratios are large.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Sudip Mandal, Lakshmi Pradeep Chitta, Patrick Antolin, Hardi Peter, Sami K. Solanki, Frederic Auchere, David Berghmans, Andrei N. Zhukov, Luca Teriaca, Regina A. Cuadrado, Udo Schuehle, Susanna Parenti, Eric Buchlin, Louise Harra, Cis Verbeeck, Emil Kraaikamp, David M. Long, Luciano Rodriguez, Gabriel Pelouze, Conrad Schwanitz, Krzysztof Barczynski, Phil J. Smith
Summary: This study investigates the phenomena of decayless kink oscillations in active-region coronal loops. High-resolution observations from two different instruments are used to compare the resolved wave activities. The results suggest that supergranular flows, which are often thought to be the drivers of these oscillations, may not be the primary factor. The analysis also casts doubt on other proposed wave drivers, indicating the need for further research in this area.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Multidisciplinary Sciences
Alessandro Bemporad
Summary: Due to the lack of UV-EUV observations of CMEs far from the Sun, our understanding of the thermodynamic evolution of these solar phenomena is limited. This study analyzed a slow CME observed in visible and UV light and used the data to determine the distribution of plasma electron density, temperature, and thermal energy. The results showed that the CME core had higher temperatures compared to the surrounding void and front, and the core temperatures increased during the CME expansion, indicating plasma heating processes. The distribution of thermal energy also exhibited asymmetry, possibly due to interaction with nearby coronal structures. This work demonstrates the potential of combining UV and visible light data and future multi-slit spectroscopic observations of CMEs.
Article
Astronomy & Astrophysics
Rebecca A. Robinson, Mats Carlsson
Summary: Numerical models can provide context to observations of nanoflare-scale reconnection events and help determine the details of these events. Detecting and understanding the mechanisms behind small-scale reconnection events is crucial for studying solar activity.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Sargam M. Mulay, Durgesh Tripathi, Helen Mason, Giulio Del Zanna, Vasilis Archontis
Summary: We studied the temperature structure of plasmoids in recurrent active region jets. Using EUV/UV images and X-ray images, we observed multithermal plasmoids travelling along the spire and footpoint region of the jets. The brightness, electron number densities, and peak temperatures of the spire plasmoid showed a systematic rise and fall during propagation. The plasmoids at the footpoint and spire had similar peak temperatures but different DEM weighted temperatures.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
M. Broese, A. Warmuth, T. Sakao, Y. Su
Summary: This article investigates whether the cooling times observed in different subregions of solar flares are in accordance with existing cooling models, and whether the temperature and emission measure of certain flows differ from their surroundings. The study finds that the observed cooling times are longer than predicted, and the flows have different temperature characteristics and lower density compared to their surroundings.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Stefan Purkhart, Astrid M. Veronig
Summary: This study investigates nanoflares in the quiet-Sun regions during solar cycle 24 and finds that their energy distribution follows a power law. The contribution of nanoflares to coronal heating remains constant throughout the solar cycle.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Engineering, Aerospace
C. Mac Cormack, M. Lopez Fuentes, C. H. Mandrini, D. Lloveras, A. M. Vasquez
Summary: In this study, a differential emission measure tomographic technique was used to reconstruct the three-dimensional distribution of the thermal properties of the solar corona plasma. By combining this technique with extrapolations of the global coronal magnetic field, the coronal loops were reconstructed and the energy input required to maintain their temperature was obtained. The study found that the thermal properties of the loops were related to their lengths, and short impulsive heating events produced better results compared to constant heating.
ADVANCES IN SPACE RESEARCH
(2022)
Article
Astronomy & Astrophysics
Aishawnnya Sharma, Durgesh Tripathi
Summary: We studied the variation of temperature and non-thermal velocity with height in fan loops using observations recorded by the Extreme Ultraviolet Imaging Spectrometer onboard Hinode. We estimated the temperatures of different coronal fan loops using the emission measure (EM)-loci method and computed the non-thermal velocities. The study provides important insights into the dynamics of heating of the solar atmosphere.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
L. P. Chitta, H. Peter, P. R. Young
Summary: The study explores transient burst phenomena in the quiet solar corona using high-resolution EUV imagery, finding that the distribution of burst lifetimes peaks at around 120 seconds with a significant number of events lasting less than 60 seconds. The estimated rate of new bursts appearing on the whole Sun is about 100 per second, but these bursts do not play a significant role in heating the solar corona.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
H. Peter, E. Alsina Ballester, V. Andretta, F. Auchere, L. Belluzzi, A. Bemporad, D. Berghmans, E. Buchlin, A. Calcines, L. P. Chitta, K. Dalmasse, T. del Pino Aleman, A. Feller, C. Froment, R. Harrison, M. Janvier, S. Matthews, S. Parenti, D. Przybylski, S. K. Solanki, J. Stepan, L. Teriaca, J. Trujillo Bueno
Summary: The magnetic activity of the Sun affects Earth and human life directly, and can also impact the habitability of planets orbiting other stars. Lack of direct information on the magnetic field in the higher atmospheric layers of the Sun hampers progress in understanding solar magnetic activity. New instruments with enhanced capabilities have been proposed to address fundamental questions and advance our understanding of the Sun and the heliosphere.
EXPERIMENTAL ASTRONOMY
(2022)
Article
Astronomy & Astrophysics
H. Bretonniere, M. Huertas-Company, A. Boucaud, F. Lanusse, E. Jullo, E. Merlin, D. Tuccillo, M. Castellano, J. Brinchmann, C. J. Conselice, H. Dole, R. Cabanac, H. M. Courtois, F. J. Castander, P. A. Duc, P. Fosalba, D. Guinet, S. Kruk, U. Kuchner, S. Serrano, E. Soubrie, A. Tramacere, L. Wang, A. Amara, N. Auricchio, R. Bender, C. Bodendorf, D. Bonino, E. Branchini, S. Brau-Nogue, M. Brescia, V. Capobianco, C. Carbone, J. Carretero, S. Cavuoti, A. Cimatti, R. Cledassou, G. Congedo, L. Conversi, Y. Copin, L. Corcione, A. Costille, M. Cropper, A. Da Silva, H. Degaudenzi, M. Douspis, F. Dubath, C. A. J. Duncan, X. Dupac, S. Dusini, S. Farrens, S. Ferriol, M. Frailis, E. Franceschi, M. Fumana, B. Garilli, W. Gillard, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, S. V. H. Haugan, W. Holmes, F. Hormuth, P. Hudelot, K. Jahnke, S. Kermiche, A. Kiessling, M. Kilbinger, T. Kitching, R. Kohley, M. Kuemmel, M. Kunz, H. Kurki-Suonio, S. Ligori, P. B. Lilje, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovic, F. Marulli, R. Massey, S. Maurogordato, M. Melchior, M. Meneghetti, G. Meylan, M. Moresco, B. Morin, L. Moscardini, E. Munari, R. Nakajima, S. M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, V. Pettorino, S. Pires, M. Poncet, L. Popa, L. Pozzetti, F. Raison, R. Rebolo, J. Rhodes, M. Roncarelli, E. Rossetti, R. Saglia, P. Schneider, A. Secroun, G. Seidel, C. Sirignano, G. Sirri, L. Stanco, J. -L. Starck, P. Tallada-Crespi, A. N. Taylor, I. Tereno, R. Toledo-Moreo, F. Torradeflot, E. A. Valentijn, L. Valenziano, Y. Wang, N. Welikala, J. Weller, G. Zamorani, J. Zoubian, M. Baldi, S. Bardelli, S. Camera, R. Farinelli, E. Medinaceli, S. Mei, G. Polenta, E. Romelli, M. Tenti, T. Vassallo, A. Zacchei, E. Zucca, C. Baccigalupi, A. Balaguera-Antolinez, A. Biviano, S. Borgani, E. Bozzo, C. Burigana, A. Cappi, C. S. Carvalho, S. Casas, G. Castignani, C. Colodro-Conde, J. Coupon, S. de la Torre, M. Fabricius, M. Farina, P. G. Ferreira, P. Flose-Reimberg, S. Fotopoulou, S. Galeotta, K. Ganga, J. Garcia-Bellido, E. Gaztanaga, G. Gozaliasl, I. M. Hook, B. Joachimi, V. Kansal, A. Kashlinsky, E. Keihanen, C. C. Kirkpatrick, V. Lindholm, G. Mainetti, D. Maino, R. Maoli, M. Martinelli, N. Martinet, H. J. McCracken, R. B. Metcalf, G. Morgante, N. Morisset, J. Nightingale, A. Nucita, L. Patrizii, D. Potter, A. Renzi, G. Riccio, A. G. Sanchez, D. Sapone, M. Schirmer, M. Schultheis, V. Scottez, E. Sefusatti, R. Teyssier, I. Tutusaus, J. Valiviita, M. Viel, L. Whittaker, J. H. Knapen
Summary: We present a machine learning framework to simulate more realistic galaxies for the Euclid Survey. The proposed method combines control on galaxy shape parameters from analytic models with realistic surface brightness distributions learned from real observations. Based on simulations, the researchers estimate that the Euclid Survey will be able to resolve internal morphological structure of galaxies and provide a complete sample of approximately 250 million galaxies.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
A. Dolliou, S. Parenti, F. Auchere, K. Bocchialini, G. Pelouze, P. Antolin, D. Berghmans, L. Harra, D. M. Long, U. Schuehle, E. Kraaikamp, K. Stegen, C. Verbeeck, S. Gissot, R. Aznar Cuadrado, E. Buchlin, M. Mierla, L. Teriaca, A. N. Zhukov
Summary: On May 30, 2020, small and short-lived extreme-UV (EUV) brightenings in the quiet Sun were observed, and their physical origin and possible impact on coronal or transition region (TR) heating are still unknown. This study aims to derive the statistical thermal evolution of these events in order to establish their coronal or transition region origin.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
F. Auchere, E. Soubrie, G. Pelouze, E. Buchlin
Summary: This study aimed to develop a general purpose image enhancement technique that produces equally good results based on an objective criterion. The method equalizes the power in the wavelet spectrum of the input image and uses a modified wavelet transform to suppress undesirable halos caused by data discontinuities. The proposed filter produces sharp and contrasted output without manual parameter adjustment and prevents high-frequency noise without smoothing significant small-scale features. Comparisons with other methods suggest that the whitening principle corresponds to the subjective criterion of most users when adjusting free parameters.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
Werner Curdt, Klaus Wilhelm, Udo Schuehle, Jean-Claude Vial, Philippe Lemaire, Karine Bocchialini
Summary: This article presents a revised version of the SUMER spectral atlas, with new identifications for over 100 emission lines. The solar emission curve in the SUMER spectral range is now available in digital format as supplementary material.
Article
Astronomy & Astrophysics
Gabriel Pelouze, Tom Van Doorsselaere, Konstantinos Karampelas, Julia M. Riedl, Timothy Duckenfield
Summary: Transverse oscillations of kink waves are found to experience a cutoff in the transition region, preventing them from reaching the corona. However, waves with shorter periods can still propagate to the corona with little attenuation, resulting in heating.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
C. Froment, O. V. Agapitov, V. Krasnoselskikh, S. Karbashewski, T. Dudok de Wit, A. Larosa, L. Colomban, D. Malaspina, M. Kretzschmar, V. K. Jagarlamudi, S. D. Bale, J. W. Bonnell, F. S. Mozer, M. Pulupa
Summary: The study aims to investigate the parameters of whistler waves in the young solar wind using the Parker Solar Probe (PSP). The results show that most of the detected wave packets in the cross-spectra are quasi-parallel to the background magnetic field, but a significant portion of the waves have oblique wave normal angles. It is concluded that magnetic dips provide favorable conditions for the generation of whistler waves.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
S. Karbashewski, O. V. Agapitov, H. Y. Kim, F. S. Mozer, J. W. Bonnell, C. Froment, T. Dudok de Wit, Stuart D. D. Bale, D. Malaspina, N. E. Raouafi
Summary: Observations by the Parker Solar Probe reveal intense plasma wave bursts in the young solar wind, often accompanied by inhomogeneities in the magnetic field. These waves, identified as electromagnetic whistler waves, propagate in different directions and experience significant Doppler frequency shifts. They have peak amplitudes exceeding 2 nT and represent up to 10% of the background magnetic field. We evaluate their properties, estimate the length of PSP electric field antennas at whistler frequencies, and discuss their generation mechanism.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Seray Sahin, Patrick Antolin, Clara Froment, Thomas A. Schad
Summary: Coronal rain is a phenomenon of colder and denser material in the solar corona, which is closely related to coronal heating. It is found that coronal rain is widespread in active regions, regardless of the inclination of the loops, and shows minimal variation during observation. Most coronal rain has a downward trajectory, but upward motions are also common. Furthermore, long-period EUV intensity pulsations are ubiquitous in active regions, and short-term periodicity (16 minutes) linked to the appearance of coronal rain poses a challenge to the thermal nonequilibrium-thermal instability scenario.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Mingzhe Guo, Timothy Duckenfield, Tom Van Doorsselaere, Konstantinos Karampelas, Gabriel Pelouze, Yuhang Gao
Summary: We simulate a magnetic cylinder in the solar atmosphere, extending from the chromosphere to the corona. Kink oscillations are launched in the loop, causing heating through the dissipation of wave energy from the Kelvin-Helmholtz instability. The coronal counterpart of the driven loop shows increased temperature and internal energy. Chromospheric evaporation is observed due to thermal conduction. Despite slight changes in average temperature and density (around 4% relative to a non-driven loop), the redistribution of density and temperature by enthalpy flow enhances wave energy dissipation in the corona. The efficient heating in the coronal counterpart of the loop complements thermal conductive losses, maintaining internal energy in the corona.
ASTROPHYSICAL JOURNAL LETTERS
(2023)
Article
Astronomy & Astrophysics
M. Janvier, S. Mzerguat, P. R. Young, E. Buchlin, A. Manou, G. Pelouze, D. M. Long, L. Green, A. Warmuth, F. Schuller, P. Demoulin, D. Calchetti, F. Kahil, L. Bellot Rubio, S. Parenti, S. Baccar, K. Barczynski, L. K. Harra, L. A. Hayes, W. T. Thompson, D. Mueller, D. Baker, S. Yardley, D. Berghmans, C. Verbeeck, P. J. Smith, H. Peter, R. Aznar Cuadrado, S. Musset, D. H. Brooks, L. Rodriguez, F. Auchere, M. Carlsson, A. Fludra, D. Hassler, D. Williams, M. Caldwell, T. Fredvik, A. Giunta, T. Grundy, S. Guest, E. Kraaikamp, S. Leeks, J. Plowman, W. Schmutz, U. Schuehle, S. D. Sidher, L. Teriaca, S. K. Solanki, J. C. del Toro Iniesta, J. Woch, A. Gandorfer, J. Hirzberger, D. Orozco Suarez, T. Appourchaux, G. Valori, J. Sinjan, K. Albert, R. Volkmer
Summary: The Solar Orbiter mission completed its first remote-sensing observation windows in the spring of 2022, providing an unprecedented view of a flaring region with a large range of observations. This study aims to understand the nature of the flaring and filament eruption events and compares the observed features with the predictions given by the standard flare model in 3D.
ASTRONOMY & ASTROPHYSICS
(2023)