Results 61 to 70 of about 41,638 (224)

Synthesis of 3-D coronal-solar wind energetic particle acceleration modules [PDF]

, 2014
1. Introduction Acute space radiation hazards pose one of the most serious risks to future human and robotic exploration. Large solar energetic particle (SEP) events are dangerous to astronauts and equipment.
Chandran, Benjamin D.G., Cooper, J. F., Desai, M., Downs, Cooper, Germaschewski, Kai K., Giacalone, Joe, Gorby, Matthew J., Isenberg, Philip A., Kasper, J. C., Korreck, K. E., Kozarev, K., Lee, Martin A., Linker, J. A., Lionello, Roberto, Lugaz, Noe E., MacNeice, Peter, Mikic, Z., Riley, P., Schwadron, Nathan A., Smith, Sonya S., Spence, Harlan E., Stevens, M. L., Torak, Tibor   +22 more
core   +2 more sources

Radio Interference Prediction Method for EHV AC Transmission Lines at High Altitudes Based on Long‐Term Observations

High Voltage, EarlyView.
ABSTRACT Radio interference (RI) is a critical factor in the design of extra‐high voltage (EHV) transmission lines at high altitudes. To address the insufficient field data of RI on high‐altitude transmission lines, the lack of adequate validation for existing RI prediction methods, and the difficulty in assessing RI levels under various meteorological
Yemao Zhang, Baoquan Wan, Yao Lu, Xingfa Liu, Bing Zhou, Jilai Xu, Hao Wan   +6 more
wiley   +1 more source

The International Guideline for the Definition, Classification, Diagnosis and Management of Urticaria

Allergy, EarlyView.
ABSTRACT This update and revision of the international guideline for urticaria was developed in accordance with the methods recommended by Cochrane and the Grading of Recommendations Assessment, Development and Evaluation (GRADE) working group. It is an initiative of the Global Allergy and Asthma Excellence Network (GA2LEN) and its Urticaria and ...
T. Zuberbier, Z. Abdul Hameed Ansari, A. H. Abdul Latiff, M. M. Abuzakouk, M. S. Agcaoili‐De Jesus, R. C. Agondi, M. Al‐Ahmad, A. A. Alangari, H. Alhameli, C. D. Alonso Bello, S. Alshareef, S. Al‐Tamemi, S. Altrichter, H. Al Wahshi, S. Aquilina, M. Araújo, R. Arnaout, R. Asero, B. Ballmer‐Weber, C. Bangert, A. Bauer, M. Ben‐Shoshan, J. A. Bernstein, C. Bindslev‐Jensen, M. Bizjak, I. Boccon‐Gibod, H. Bonnekoh, L. Bouillet, K. Brockow, Z. Brzoza, M. Bulatović Ćalasan, A. Bulkhi, T. Buttgereit, A. Bygum, T. Caballero, O. Calderon, R. Campos, M. Cancian, E. Carne, M. A. Castor, I. Cerecedo, T. Çetinarslan, I. Cherrez‐Ojeda, N. Chkhikvadze, H. J. Chong‐Neto, K. Choo, G. Christoff, C.‐Y. Chu, K. Ciupka, N. Conlon, C. Costa, T. Craig, P. Criado, I. Danilycheva, R. Darlenski, E. De Arruda Chaves, L. de Montjoye, M. S. Doutre, A. Du‐Thanh, D. Ebo, S. Elkhalifa, S. Elmariah, T. El‐Shanawany, L. F. Ensina, R. Ertaş, R. Fachini Jardim Criado, M. Ferrer, S. Ferrucci, J. S. Fok, D. Fomina, L. Fonacier, G. Fouda, I. Francescantonio, A. Fukunaga, C. A. Galvan Calle, E. Garcia, K. Gáspár, A. Gelincik, S. Geng, K. Godse, M. Gonçalo, M. Gotua, C. Grattan, M. Grosber, G. Guidos Fogelbach, M. Guilarte, R. Guillod, E. Hamelmann, J. Hawkes, K. Hayama, R. Heuer, M. Hide, W. Hoetzenecker, N. Inomata, H.‐R. Kang, A. Kaplan, A. Kapp, M. Karam, A. Kasperska‐Zajac, C. H. Katelaris, A. Kessel, M. Khoshkhui, B. Kim, T. Kinaciyan, E. Kocatürk, M. Kolacinska‐Flont, P. Kolkhir, G. N. Konstantinou, M. Kosnik, D. Krasowska, K. Kulthanan, M. S. Kumaran, I. Kuprys‐Lipinska, M. Labrador, J. I. Larco, D. Larenas‐Linnemann, E. Latysheva, E. Lazaridou, P. H. Li, H. Lima, U. Lippert, M. Magerl, M. Makris, J. Alves Marcelino, A. V. Marzano, I. Medina, R. Meshkova, D. Micallef, R. Mohammed Ali, C. G. Mortz, M. Munoz, H. N. G. Oude Elberink, A. Nakonechna, I. Nasr, A. Nast, E. Netchiporouk, E. Nettis, S. Nieto, I. Ogueta Canales, T.‐L. Okas, R. L. Orfali, E. Özkaya, C. Parisi, A. Pennitz, R. Pawankar, M. P. Pereira, J. Peter, E. Petkova, P. D. Pigatto, I. Podder, T. Popov, G. Porebski, P. Pyatilova, G. D. Ramon, H. A. Ratti Sisa, M. Recto, K. Ress, K. Ridge, M. Riedl, C. Ritchie, N. Rosario Filho, I. Rosmaninho, M. Rudenko, M. Rukhadze, K. Rutkowski, V. Sabato, U. M. Sahiner, S. Saini, F. Saleh Al Sabbagh, A. Salman, F. Salvo, J. Sanchez, A. Santucci, S. Schliemann, P. Schmid‐Grendelmeier, B. E. Sekerel, F. Serpa, F. Sheikh, J. Sheikh, H. Shendi, F. Siebenhaar, M. Sonomjamts, A. Soria, B. Sousa Pinto, M. Staevska, P. Staubach, M. Stephan, K. Stevanovic, L. Stingeni, M. Stobiecki, Ö. Su Küçük, G. Sussman, A. Szegedi, S. Takahagi, A. Tanaka, N. Teovska Mitrevska, S. F. Thomsen, E. Toubi, F. Tsatsou, M. Turk, Z. Vadasz, A. Valerieva, S. Valle, M. v. Doorn, B. Veleiro Perez, C. E. Vera Ayala, C. Vestergaard, R. J. Vieira, C. W. Maruta, B. Wedi, R. N. Werner, E. W. Y. Yap, P. Xepapadaki, Y. Xiang, Y.‐M. Ye, P. Yong, G. Yosipovitch, A. Z. J. Zalewska‐Janowska, C. Zeyen, Z. Zhao, M. Metz, A. M. Giménez‐Arnau   +221 more
wiley   +1 more source

On the Origin of the Dominant Waves in the Extended Solar Corona

The Astrophysical Journal
The extended solar corona at 10–30 solar radii is essentially devoid of all waves below 100 kHz other than triggered ion acoustic waves (TIAWs), which consist of a low-frequency (LF) electromagnetic wave at a frequency of a few Hz coupled to one or more ...
F. S. Mozer, O. V. Agapitov, O. Romeo, V. Roytershteyn, A. Voshchepynets   +4 more
doaj   +1 more source

New views on the emission and structure of the solar transition region

, 2010
The Sun is the only star that we can spatially resolve and it can be regarded as a fundamental plasma laboratory of astrophysics. The solar transition region (TR), the layer between the solar chromosphere and corona, plays an important role in solar wind
Aiouaz, Aiouaz, Athay, Athay, Axford, Bartoe, Bartoe, Bartoe, Basri, Bocchialini, Bohlin, Bonnet, Brekke, Brosius, Brosius, Brosius, Brown, Brueckner, Brueckner, Brueckner, Brynildsen, Büchner, Büchner, Chae, Chae, Chae, Chen, Chen, Chen, Chuanyi Tu, Culhane, Curdt, Curdt, Curdt, Curdt, Curdt, Curdt, Dammasch, Dammasch, De Pontieu, Del Zanna, Dere, Dere, Dere, Doschek, Doschek, Doschek, Dowdy, Doyle, Doyle, Doyle, Doyle, Eckart Marsch, Evershed, Evershed, Falconer, Fang, Feldman, Feldman, Feldman, Fontenla, Fontenla, Foukal, Foukal, Foukal, Gabriel, Golub, Gontikakis, Gouttebroze, Gouttebroze, Griffiths, Gunár, Guo, Habbal, Hansteen, Hansteen, Harra, Harrison, Harrison, Hassler, He, He, He, Heinzel, Hui Tian, Hénoux, Ichimoto, Imada, Innes, Innes, Jiansen He, Jin, Jordan, Katsukawa, Kneer, Lemaire, Lemaire, Lemaire, Li, Liu, Longcope, Madjarska, Madjarska, Magara, Mariska, Mariska, Marsch, Marsch, Marsch, Marsch, Marsch, Marsch, McClymont, McIntosh, McIntosh, McIntosh, McIntosh, Metcalf, Nicolas, Nicolas, Parnell, Patsourakos, Peter, Peter, Peter, Peter, Peter, Popescu, Priest, Raju, Ravindra, Reeves, Sakao, Santos, Schmieder, Schrijver, Seehafer, Sheeley, Solanki, Stucki, Teriaca, Teriaca, Teriaca, Teriaca, Teriaca, Teriaca, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tu, Tu, Tu, Ugarte-Urra, Ugarte-Urra, Ugarte-Urra, Vernazza, Vernazza, Vial, Vial, Vial, Wang, Wang, Warren, Watanabe, Webb, Werner Curdt, Wiegelmann, Wiegelmann, Wiegelmann, Wilhelm, Wilhelm, Wilhelm, Wilhelm, Wilhelm, Xia, Xia, Xia, Xu, Zhang, Zhang, Zhang, Zhang, Zhang, Zhang   +192 more
core   +1 more source

Long-period intensity pulsations in the solar corona during activity cycle 23 [PDF]

Astronomy & Astrophysics, 2014
We report on the detection (10 ) of 917 events of long-period (3 to 16 hours) intensity pulsations in the 19.5 nm passband of the SOHO Extreme ultraviolet Imaging Telescope. The data set spans from January 1997 to July 2010, i.e the entire solar cycle 23 and the beginning of cycle 24.
Auchère, F., Bocchialini, K., Solomon, J., Tison, E.   +3 more
openaire   +2 more sources

Observational Test of Coronal Magnetic Field Models I. Comparison with Potential Field Model

, 2008
Recent advances have made it possible to obtain two-dimensional line-of-sight magnetic field maps of the solar corona from spectropolarimetric observations of the Fe XIII 1075 nm forbidden coronal emission line.
Arnaud J., Haosheng Lin, Liu Y., Yu Liu
core   +1 more source

Observation of coronal loop torsional oscillation [PDF]

, 2003
We suggest that the global torsional oscillation of solar coronal loop may be observed by the periodical variation of a spectral line width. The amplitude of the variation must be maximal at the velocity antinodes and minimal at the nodes of the ...
Zaqarashvili, T. V.
core   +3 more sources

Understanding the Evidence Gaps: Diets and Fruit and Vegetable Intake Across Five Diverse Low‐ and Middle‐Income Countries

Maternal &Child Nutrition, EarlyView.
This perspective article synthesizes findings from scoping reviews examining diet and F&V intake, and interventions to increase F&V consumption among population groups in five countries: Benin, Fiji, the Philippines, Sri Lanka and Tanzania. ABSTRACT Poor dietary quality, particularly inadequate fruit and vegetable (F&V) intake, remains a significant ...
Manisha Tharaney, Sonja Y. Hess, Lilia Bliznashka, Dorcas A. Amunga, Fusta Azupogo, Nadia Koyratty, Taryn J. Smith, Imelda Angeles‐Agdeppa, Eva A. Goyena, Frederick Grant, Joyce Kinabo, Irene Medeme Mitchodigni, Anasaini Moala Silatolu, Renuka Silva, Mutinta Hambayi, Thushanthi Perera, Deanna K. Olney   +16 more
wiley   +1 more source

Nonlinear Fast Magnetosonic Waves in Solar Prominence Pillars

The Astrophysical Journal, 2023
We investigate the properties of nonlinear fast magnetosonic (NFM) waves in a solar prominence, motivated by recent high-resolution and high-cadence Hinode/Solar Optical Telescope (SOT) observations of small-scale oscillations in a prominence pillar.
Leon Ofman, Therese A. Kucera, C. Richard DeVore   +2 more
doaj   +1 more source