The first widespread solar energetic particle event observed by Solar Orbiter on 2020 November 29

Context. On 2020 November 29, the first widespread solar energetic particle (SEP) event of solar cycle 25 was observed at four widely separated locations in the inner (. 1 AU) heliosphere. Relativistic electrons as well as protons with energies > 50 MeV were observed by Solar Orbiter (SolO), Parker Solar Probe (PSP), the Solar Terrestrial Relations Observatory (STEREO)-A and multiple near-Earth spacecraft. The SEP event was associated with an M4.4 class X-ray flare and accompanied by a coronal mass ejection (CME) and an extreme ultraviolet (EUV) wave as well as a type II radio burst and multiple type III radio bursts. Aims. We present multi-spacecraft particle observations and place them in context with source observations from remote sensing instruments and discuss how such observations may further our understanding of particle acceleration and transport in this widespread event. Methods. Velocity dispersion analysis (VDA) and time shift analysis (TSA) were used to infer the particle release times at the Sun. Solar wind plasma and magnetic field measurements were examined to identify structures that influence the properties of the energetic particles such as their intensity. Pitch angle distributions and first-order anisotropies were analyzed in order to characterize the particle propagation in the interplanetary medium. Results. We find that during the 2020 November 29 SEP event, particles spread over more than 230° in longitude close to 1 AU. The particle onset delays observed at the different spacecraft are larger as the flare–footpoint angle increases and are consistent with those from previous STEREO observations. Comparing the timing when the EUV wave intersects the estimated magnetic footpoints of each spacecraft with particle release times from TSA and VDA, we conclude that a simple scenario where the particle release is only determined by the EUV wave propagation is unlikely for this event. Observations of anisotropic particle distributions at SolO, Wind, and STEREO-A do not rule out that particles are injected over a wide longitudinal range close to the Sun. However, the low values of the first-order anisotropy observed by near-Earth spacecraft suggest that diffusive propagation processes are likely involve

Recommendations for the Implementation of the Self-Administration of Alpha-1 Antitrypsin

María Torres-Durán,1 José Luis López-Campos,2,3 Myriam Calle Rubio,4 Carmen Montero-Martínez,5 Ana Priegue Carrera,6 Rosanel Amaro Rodríguez,7 Miriam Barrecheguren,8 María Ángeles Barrio Guirado,9 Francisco Javier Callejas-González,10 Francisco Casas-Maldonado,11 Layla Diab-Cáceres,12 Pilar García-Meseguer,9 José María Hernández-Pérez,13 Lourdes Lázaro-Asegurado,14 Cristina Martínez-González,15 Carlos Martínez Rivera,16 Francisco Javier Michel,17 José-Bruno Montoro-Ronsano,18 Raquel Sánchez,19 Marta Ortiz-Pica,20 Isabel Parra,21 José Pablo Quintero García,22 María del Rosario Ruiz-Serrano-de la Espada,23 Begoña Tortajada-Goitia,24 Marc Miravitlles8 1Pneumology Department, Hospital Álvaro Cunqueiro, NeumoVigo I+i Research Group, IIS Galicia Sur, Vigo, Spain; 2Instituto de Salud Carlos III, Centro de Investigación Biomédica en Red de Enfermedades Respiratorias (CIBERES), Madrid, Spain; 3Medical and Surgery Unit for Respiratory Diseases, Instituto de Biomedicina de Sevilla (IBiS), Hospital Universitario Virgen del Rocío/Universidad de Sevilla, Seville, Spain; 4Pneumology Department, Research Institute of Hospital Clínico San Carlos (IdISSC), Department of Medicine, Faculty of Medicine, University Complutense of Madrid, Madrid, Spain; 5Pneumology Department, Hospital Universitario de A Coruña, A Coruña, Spain; 6Nursing Unit, Hospital Álvaro Cunqueiro, Pontevedra, Spain; 7Pneumology Department, Hospital Clínic, Barcelona, Spain; 8Pneumology Department, Hospital Universitari Vall d’Hebron, Vall d’Hebron Institut de Recerca (VHIR), Vall d’Hebron Barcelona Hospital Campus, Barcelona, Spain; 9Nursung Unit, Hospital Universitari Vall d’Hebron, Barcelona, Spain; 10Pneumology Department, Complejo Hospitalario Universitario de Albacete, Albacete, Spain; 11Pneumology Department, Hospital Universitario Clínico San Cecilio, Granada, Spain; 12Pneumology Department, Hospital Universitario 12 de Octubre, Madrid, Spain; 13Pneumology Department, Hospital Universitario Nuestra Señora de La Candelaria, Santa Cruz de Tenerife, Tenerife, Spain; 14Pneumology Department, Complejo Asistencial Universitario de Burgos, Burgos, Spain; 15Instituto de Investigación Sanitaria del Principado de Asturias (FINBA-ISPA) Oviedo, Oviedo, Spain; 16Pneumology Department, Hospital Universitario Germans Trías I Pujol, Institut d’investigació Germans Trias i Pujol (IGTP), Badalona, Spain; 17Pneumology Department, Hospital Universitario Donostia, Donostia, Spain; 18Hospital Pharmacy Department, Hospital Universitari Vall d’Hebron, Vall d’Hebron Barcelona Hospital Campus, Barcelona, Spain; 19Pneumology Department, Hospital Universitario Basurto, Bilbao, Spain; 20Nursing Unit, Hospital Clínico San Carlos, Madrid, Spain; 21Pneumology Department, Hospital Clínico Universitario Virgen de la Arrixaca, Murcia, Spain; 22Hospital Pharmacy Department, Hospital Universitario Virgen del Rocío, Sevilla, Spain; 23Nursing Unit, Hospital Universitario Virgen del Rocío, Sevilla, Spain; 24Hospital Pharmacy Department, Hospital Costa del Sol, Málaga, SpainCorrespondence: María Torres-Durán, Tel +34986811111, Email [email protected]: Administration of exogenous alpha-1 antitrypsin (AAT) is the only specific therapy for the management of pulmonary morbidity in patients with AAT deficiency. It requires weekly or biweekly intravenous infusions, which may impact patient independence and quality of life. Self-administration of AAT therapy is an alternative to reduce the burden for patients who require AAT therapy. We presented herein experts’ recommendations for the implementation of a program for the self-administration of AAT.Methods: This project was conducted using a modified nominal group technique and was undertaken in two online meetings involving the participation of 25 experts: specialists in pulmonology (n=17), nurses (n=5) and hospital pharmacists (n=3).Results: The following issues were discussed, and several recommendations were agreed upon on the following topics: a) patient profile and clinical evaluation, establishing selection criteria that should include clinical as well as social criteria; b) role of health care professionals, suggested roles for specialists in pulmonology, nurses, and hospital pharmacists; c) training by the nurse, including recommendations before initiating the training and the content of the training sessions; and d) logistic issues and follow-up, adherence, and patient support.Conclusion: We expect this proposal to increase awareness of this therapeutic alternative and facilitate the implementation of self-administration programs, thus contributing to optimizing the patient experience with AAT therapy. Further research on the outcomes of these programs, especially from the patient perspective, will also help to improve their design and implementation.Keywords: alpha-1 antitrypsin deficiency, disease burden, augmentation therapy, self-administratio

The first widespread solar energetic particle event observed by Solar Orbiter on 2020 November 29

Context. On 2020 November 29, the first widespread solar energetic particle (SEP) event of solar cycle 25 was observed at four widely separated locations in the inner (less than or similar to 1AU) heliosphere. Relativistic electrons as well as protons with energies >50MeV were observed by Solar Orbiter (SolO), Parker Solar Probe, the Solar Terrestrial Relations Observatory (STEREO)-A and multiple near-Earth spacecraft. The SEP event was associated with an M4.4 class X-ray flare and accompanied by a coronal mass ejection and an extreme ultraviolet (EUV) wave as well as a type II radio burst and multiple type III radio bursts. Aims. We present multi-spacecraft particle observations and place them in context with source observations from remote sensing instruments and discuss how such observations may further our understanding of particle acceleration and transport in this widespread event. Methods. Velocity dispersion analysis (VDA) and time shift analysis (TSA) were used to infer the particle release times at the Sun. Solar wind plasma and magnetic field measurements were examined to identify structures that influence the properties of the energetic particles such as their intensity. Pitch angle distributions and first-order anisotropies were analyzed in order to characterize the particle propagation in the interplanetary medium. Results. We find that during the 2020 November 29 SEP event, particles spread over more than 230 degrees in longitude close to 1AU. The particle onset delays observed at the different spacecraft are larger as the flare-footpoint angle increases and are consistent with those from previous STEREO observations. Comparing the timing when the EUV wave intersects the estimated magnetic footpoints of each spacecraft with particle release times from TSA and VDA, we conclude that a simple scenario where the particle release is only determined by the EUV wave propagation is unlikely for this event. Observations of anisotropic particle distributions at SolO, Wind, and STEREO-A do not rule out that particles are injected over a wide longitudinal range close to the Sun. However, the low values of the first-order anisotropy observed by near-Earth spacecraft suggest that di ffusive propagation processes are likely involved.Peer reviewe

Solar energetic particle heavy ion properties in the widespread event of 2020 November 29

Context. Following a multi-year minimum of solar activity, a solar energetic particle event on 2020 Nov. 29 was observed by multiple spacecraft covering a wide range of solar longitudes including ACE, the Solar Terrestrial Relations Observatory-A, and the recently launched Parker Solar Probe and Solar Orbiter. Aims. Multi-point observations of a solar particle event, combined with remote-sensing imaging of flaring, shocks, and coronal mass ejections allows for a global picture of the event to be synthesized, and made available to the modeling community to test, constrain, and refine models of particle acceleration and transport according to such parameters as shock geometries and particle mass-to-charge ratios. Methods. Detailed measurements of heavy ion intensities, time dependence, fluences, and spectral slopes provided the required test data for this study. Results. The heavy ion abundances, timing, and spectral forms for this event fall well within the range found in prior surveys at 1 au. The spectra were well fitted by broken power law shapes; the Fe/O ratio was somewhat lower than the average of other events. In addition, 3He/4He was very low, with only the upper limits established here. © 2021 ESO.Immediate accessThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at [email protected]