Mapping solar magnetic fields from the photosphere to the base of the corona.

Routine ultraviolet imaging of the Sun's upper atmosphere shows the spectacular manifestation of solar activity; yet, we remain blind to its main driver, the magnetic field. Here, we report unprecedented spectropolarimetric observations of an active region plage and its surrounding enhanced network, showing circular polarization in ultraviolet (Mg ii & and Mn i) and visible (Fe i) lines. We infer the longitudinal magnetic field from the photosphere to the very upper chromosphere.

Global maps of the magnetic field in the solar corona.

Understanding many physical processes in the solar atmosphere requires determination of the magnetic field in each atmospheric layer. However, direct measurements of the magnetic field in the Sun's corona are difficult to obtain. Using observations with the Coronal Multi-channel Polarimeter, we have determined the spatial distribution of the plasma density in the corona and the phase speed of the prevailing transverse magnetohydrodynamic waves within the plasma.

[Atlantoaxial malformation as a rare cause of dysphagia and snoring].

Abnormalities of the atlantoaxial spine are very rare variants. Bony outgrowths, osteophytes, clefts and aplasia may be misinterpreted as degenerative diseases. One patient presented with intermittent dysphagia and snoring and CT and MRI scans of the cervical spine showed an accessory bone located anterior to the atlas and axis.

Intranasal administration of drugs.

Objective: To investigate how nasally applied substances distribute in the nose depending on the form of application.

Design: Observer-blinded study.

Setting: University hospital research unit.