The MMC BioBank is a Resource that Supports Biomedical Research

Mission: To provide normal and diseased annotated human biospecimens to the research community that supports discoveries leading to improved patient therapies and advances in personalized medicine.https://knowledgeconnection.mainehealth.org/lambrew-retreat-2021/1052/thumbnail.jp

Student Satisfaction and Performance in an Online Teacher Certification Program

The article presents a study which demonstrates the effectiveness of an online post baccalaureate teacher certification program developed by a Wisconsin university. The case method approach employing multiple methods and multiple data sources were used to investigate the degree to which pre-service teachers were prepared to teach. It was concluded that the study supports online delivery as an effective means of teacher preparation, but it was limited in the number of students followed into their first year of teaching

Small lightning flashes from shallow electrical storms on Jupiter

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MMC Biobank: A resource for translational research.

BioBank Director develops an Internal Investigator protocol which outlines collection logistics, sample processing, communications with clinical personnel for executing the study plan and transport of samples to MMCRI

Systematic capture of MeV electron beams by MWR

Every ~ 53 days since August 2016, Juno swings by Jupiter and as the spacecraft spins along a polar orbit, measurements of Jupiter's microwave radiation are carried out at high data rates for several hours (~ 9 hours) with the Juno Microwave Radiometer (MWR). Within ~ 6 planetary radii (Rj) and from inside/outside the magnetospheric region, the thermal and synchrotron emissions are measured at high temporal and spatial resolutions. In this paper, we present a synthesis of the spatial distributions of the microwave radiation and discuss the similarities and differences observed at six wavelengths (1.3-50 cm). In addition to the thermal emission and synchrotron radiation from Jupiter's electron belt, unexpected signatures in MWR are either systematically or sporadically reported during perijove 1 (PJ1) and PJ3-PJ6. The preliminary results of a multi-instrument analysis of radio (MWR), extreme and far-ultraviolet auroral emissions (Juno UVS), field (Juno magnetometer), keV electrons (JEDI), and background radiation signatures in Juno's ASC and SRU instruments suggest that some of these signatures are consistent with the capture by MWR of synchrotron emission radiated by MeV electron beams, which may be associated with auroral activity. We subsequently describe in detail our data analysis and effort to model the synchrotron radiation from MeV electron beams to support our findings

Planetary Atmospheres

International audienc

Planetary Atmospheres

International audienc

Planetary Atmospheres

International audienc