Parker Solar Probe Imaging of the Night Side of Venus.

We present images of Venus from the Wide-Field Imager for Parker Solar Probe (WISPR) telescope on board the Parker Solar Probe (PSP) spacecraft, obtained during PSP's third and fourth flybys of Venus on 2020 July 11 and 2021 February 20, respectively. Thermal emission from the surface is observed on the night side, representing the shortest wavelength observations of this emission ever, the first detection of the Venusian surface by an optical telescope observing below 0.8 µm. Consistent with previous observations at 1 µm, the cooler highland areas are fainter than the surrounding lowlands. The irradiances measured by WISPR are consistent with model predictions assuming a surface temperature of T = 735 K. In addition to the thermal emission, the WISPR images also show bright nightglow emission at the limb, and we compare the WISPR intensities with previous spectroscopic measurements of the molecular oxygen nightglow lines from Venus Express.

An Introduction to Reviewing Research Articles for Academic Journals.

Description Among the pillars of science is the galvanizing process of peer review. Editors of medical and scientific publications recruit specialty leaders to evaluate the quality of manuscripts. These peer reviewers help to ensure that data are collected, analyzed, and interpreted as accurately as possible, thereby moving the field forward and ultimately improving patient care. As physician-scientists, we are given the opportunity and responsibility to participate in the peer review process. There are many benefits to engaging in the peer review process including exposure to cutting-edge research, growing your connection with the academic community, and fulfilling the scholarly activity requirements of your accrediting organization. In the present manuscript, we discuss the key components of the peer review process and hope that it will serve as a primer for the novice reviewer and as a useful guide for the experienced reviewer.

Element Abundances: A New Diagnostic for the Solar Wind.

We examine the different element abundances exhibited by the closed loop solar corona and the slow speed solar wind. Both are subject to the first ionization potential (FIP) effect, the enhancement in coronal abundance of elements with FIP below 10 eV (e.g., Mg, Si, Fe) with respect to high-FIP elements (e.g., O, Ne, Ar), but with subtle differences. Intermediate elements, S, P, and C, with FIP just above 10 eV, behave as high-FIP elements in closed loops, but are fractionated more like low-FIP elements in the solar wind. On the basis of FIP fractionation by the ponderomotive force in the chromosphere, we discuss fractionation scenarios where this difference might originate. Fractionation low in the chromosphere where hydrogen is neutral enhances the S, P, and C abundances. This arises with nonresonant waves, which are ubiquitous in open field regions, and is also stronger with torsional Alfvén waves, as opposed to shear (i.e., planar) waves. We discuss the bearing these findings have on models of interchange reconnection as the source of the slow speed solar wind. The outflowing solar wind must ultimately be a mixture of the plasma in the originally open and closed fields, and the proportions and degree of mixing should depend on details of the reconnection process. We also describe novel diagnostics in ultraviolet and extreme ultraviolet spectroscopy now available with these new insights, with the prospect of investigating slow speed solar wind origins and the contribution of interchange reconnection by remote sensing.

Risk factors for Alzheimer's disease: an overview for clinical practitioners.

OBJECTIVE: To review current information on various risk factors of Alzheimer's disease (AD) for clinicians so that they may educate patients or their families in a clinical setting. DATA SOURCES: Published medical literature and research articles from MEDLINE. STUDY SELECTION: Reviews and articles from 1985 to 2003 concerning risk factors associated with AD. DATA EXTRACTION: Data on risk factors ranging from possible or controversial to well established. DATA SYNTHESIS: AD is an irreversible, progressive neurodegenerative disorder. AD is currently known to be the most common cause of dementia in the United States. Over the last several decades, different levels of risk factors associated with AD have been identified. With more information available to the public via various resources, there is greater need for clinical practitioners to provide up-to-date information on risk factors in a meaningful way. This article discusses advanced age, family history, gender, low education, apolipoprotein E e4, head injury, cardiovascular conditions, and aluminum. CONCLUSION: Since there currently is no cure or preventive measure for AD, it is important to educate patients and their families about risk factors of AD in clinical practice.

Astrospheres and Solar-like Stellar Winds.

Stellar analogs for the solar wind have proven to be frustratingly difficult to detect directly. However, these stellar winds can be studied indirectly by observing the interaction regions carved out by the collisions between these winds and the interstellar medium (ISM). These interaction regions are called "astrospheres", analogous to the "heliosphere" surrounding the Sun. The heliosphere and astrospheres contain a population of hydrogen heated by charge exchange processes that can produce enough H I Lyα absorption to be detectable in UV spectra of nearby stars from the Hubble Space Telescope (HST). The amount of astrospheric absorption is a diagnostic for the strength of the stellar wind, so these observations have provided the first measurements of solar-like stellar winds. Results from these stellar wind studies and their implications for our understanding of the solar wind are reviewed here. Of particular interest are results concerning the past history of the solar wind and its impact on planetary atmospheres.