Missing women: policing absence

This paper considers the neglected mobilities associated with a sample of UK women reported as missing.Refracted through literatures on gendered mobility and abandonment, the paper argues that the journeys of thesewomen in crisis are not well understood by police services, and that normative gender relations may infuse theirmanagement. By selectively exploring one illustrative police case file on Kim, we highlight how reported andobserved socio-spatial relationships within private and public spaces relate to search actions. We argue that Kim’smobility and spatial experiences are barely understood, except for when they appear to symbolise disorder anddanger. We address the silences in this singular case by using the voices of other women reported as missing, ascollected in a research project to explore the agency, experience and meaning of female mobility during absence.We argue that women reported as missing are not abandoned by UK policing services, but that a policy ofcontinued search for them may be at risk if they repeatedly contravene normative socio-spatial relationshipsthrough regular absence mobilities. By way of conclusion, we address recent calls for research that explores therelationships between gender and mobility.

Solar coronal jets: observations, theory, and modeling

Coronal jets represent important manifestations of ubiquitous solar transients, which may be the source of significant mass and energy input to the upper solar atmosphere and the solar wind. While the energy involved in a jet-like event is smaller than that of “nominal” solar flares and coronal mass ejections (CMEs), jets share many common properties with these phenomena, in particular, the explosive magnetically driven dynamics. Studies of jets could, therefore, provide critical insight for understanding the larger, more complex drivers of the solar activity. On the other side of the size-spectrum, the study of jets could also supply important clues on the physics of transients close or at the limit of the current spatial resolution such as spicules. Furthermore, jet phenomena may hint to basic process for heating the corona and accelerating the solar wind; consequently their study gives us the opportunity to attack a broad range of solar-heliospheric problems.