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Ionospheric Response to Geomagnetic Storms of Different Intensity in the Eastern North Atlantic Mid-Latitudinal Zone (Iberian Peninsula, Azores and Madeira): Solar and Geomagnetic Drivers
You are already at the latest version Ionospheric response to a geomagnetic storm depends on several factors. Strength of a storm, commencement type, type of the solar origin of a geomagnetic storm (e.g., coronal mass ejections or high-speed solar wind streams) and observational site location are among them.
Scintillations in Southern Europe During the Geomagnetic Storm of June 2015
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Molecular Dynamics Simulations Reveal How Competing Protein–Surface Interactions for Glycine, Citrate, and Water Modulate Stability in Antibody Fragment Formulations
Introduction Click to copy section linkSection link copied! Achieving liquid formulations that are stable for long periods during storage and transport, often at 4–8 °C, is critical to the successful development of therapeutic proteins such as antibodies and other antibody-based formats. (1−5) Protein aggregation is a major degradation pathway that can lead to loss of potency and increased risk of adverse immunogenicity.
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