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Smaller summer harmful algal bloom of 3 predicted for western Lake Erie


The Beacon
This is an algal bloom in Saginaw Bay, as seen by aircraft during a flyover in summer of 2019. This airborne campaign is ongoing in conjunction with NOAA weekly Lake Erie monitoring and biweekly sampling in Saginaw Bay. The flyovers are done in collaboration with researchers at NASA Glenn. (Zachary Haslick, Aerial Associates Photography Inc.)
The National Oceanic and Atmospheric Administration and its research partners are forecasting western Lake Erie will experience a smaller-than-average harmful algal bloom this summer of 3 on a scale of 10. A relatively dry spring will lead to a repeat of last year’s mild bloom. ....

United States , Lake Erie , Ohio State University , Mike Dewine , Richard Stumpf , Paul Scholz , Christopher Winslow , Stone Laboratory , University Of Toledo , National Centers For Coastal Ocean Science , University Of Michigan , National Oceanic , Institute For Great Lakes Research , European Union Copernicus , National Ocean Service , Carolina State University , Heidelberg University , Ohio River Forecast Center , Carnegie Institution For Science , Atmospheric Administration , Stanford University , Great Lakes Environmental Research Laboratory , Ohio Department , Higher Education , Harmful Algal Bloom Research Initiative , Ohio Sea Grant ,

Milky Way magnetar likely source of fast radio burst – Astronomy Now


An artist’s impression of a magnetar generating a high-energy flare showing the collapsed star’s complex magnetic field and a beamed polar emission. Image: McGill University Graphic Design Team
For the first time, astronomers have detected a fast radio burst, or FRB, in the Milky Way, a titanic outburst of X-rays and radio waves that was generated in a fraction of a second. Until now, FRBs were only seen in other galaxies and their sources were a mystery.
Now, astronomers at multiple institutions have pinpointed the FRB spotted in the Milky Way and conclude it most likely was generated by a magnetar, a super-magnetised neutron star with many times the mass of the Sun. The magnetic field generated by a magnetar can be a thousand times more intense than that of a typical neutron star. ....

United Kingdom , Chris Bochenek , Paul Scholz , University Of Toronto , University Of British Columbia , Canadian Hydrogen Intensity Mapping Experiment , Mcgill University , Mcgill University Graphic Design Team , Mcgill University Graphic Design , Milky Way , Dominion Radio Astrophysical Observatory , British Columbia , Dunlap Institute , ஒன்றுபட்டது கிஂக்டம் , பால் ஸ்கோல்ஸ் , பல்கலைக்கழகம் ஆஃப் டொராண்டோ , பல்கலைக்கழகம் ஆஃப் பிரிட்டிஷ் கொலம்பியா , கனடியன் ஹைட்ரஜன் தீவிரம் விவரணையாக்கம் சோதனை , மகில் பல்கலைக்கழகம் , மகில் பல்கலைக்கழகம் கிராஃபிக் வடிவமைப்பு அணி , மகில் பல்கலைக்கழகம் கிராஃபிக் வடிவமைப்பு , பால் வழி , ஆதிக்கம் வானொலி வானியற்பியல் கண்காணிப்பு , பிரிட்டிஷ் கொலம்பியா , டன்லப் நிறுவனம் ,