نتایج جستجو برای: hepatic flare
تعداد نتایج: 102107 فیلتر نتایج به سال:
We use Hinode observations to study coronal structures about to flare, based on their apparent footpoints as a guide to identification. The high resolution and excellent stability of the Hinode observations makes the identifications much more precise than those done with the soft X-ray telescope (SXT) on board Yohkoh. The physical conditions in the coronal structure about to flare are important...
The purpose of our study is to evaluate the effect of a single drop of latanoprost on the intraocular pressure and blood-aqueous barrier permeability in 8 patients with uveitis. The degree of inflammation was determined by the intensity of aqueous flare measured with a laser flare cell meter every 2 hours from 11:00 to 17:00 hours for 2 days. Intraocular pressure was measured at 11:00 and 17:00...
acute cholangitis (ac) is commonly observed in general practice with different causes. we report a case of recurrent ac caused by anomaly of the right hepatic artery, as a rare underlying condition.
We report the possible detection of a Li i λ6708 Å line enhancement during an unusual long-duration optical flare in the recently discovered, X-ray/EUV selected, chromospherically active binary 2RE J0743+224. The Li i equivalent width (EW) variations follow the temporal evolution of the flare and large changes are observed in the intensity of the line. The maximum Li i enhancement (40% in EW) o...
A laser flare-cell meter was used to examine blood-aqueous barrier function in a 21-year-old male patient who had typical retinitis punctata albescens with white dots scattered throughout large areas of the fundus in both eyes. Fluorescein angiography showed multiple areas of hyperfluorescence over dot lesions and window defects. Electroretinogram demonstrated subnormal amplitude and electroocu...
We report the possible detection of a Li i λ6708 Å line enhancement during an unusual long-duration optical flare in the recently discovered, X-ray/EUV selected, chromospherically active binary 2RE J0743+224. The Li i equivalent width (EW) variations follow the temporal evolution of the flare and large changes are observed in the intensity of the line. The maximum Li i enhancement (40% in EW) o...
Recently, the MAGIC collaboration reported evidence for a delay in the arrival times of photons of different energies during a γ-ray flare from the blazar Markarian 501 on 2005 July 9. We describe the observed delayed high-energy emission by applying a homogeneous synchrotron self-Compton (SSC) model under the assumption that the blob containing relativistic electrons was observed in its accele...
Of the many episodic variations associated with the active Sun, perhaps the solar flare is the most spectacular and enigmatic. Because flares emit photons that reach our atmosphere in about 8 minutes, with no intervening heliospheric or magneto spheric interactions, flare effects upon the geospace system have been a somewhat neglected component in Space Weather research. Once flare photons pass...
I report on the X-ray detection of Gl 569 Bab. During a 25 ksec Chandra observation the binary brown dwarf is for the first time spatially separated in X-rays from the flare star primary Gl 569 A. Companionship to Gl 569 A constrains the age of the brown dwarf pair to 300 − 800 Myr. The observation presented here is only the second X-ray detection of an evolved brown dwarf. About half of the ob...
Results The study population included 18 (13%) extended oligoarticular, 17 (12%) RF+ Poly and 102 (75%) RFPoly JIA patients. At enrollment, age (mean/median/range) was 11.3/11.6/3.4-20.1 yrs; disease duration was 5.0/4.1/0.618.6 yrs; 103 (75%) were females and 64 (47%) were ANA +. Duration of CID at baseline was 1.2/0.5/1 day-12.1 yrs. Anti-TNF was etanercept in 106 (77%), 25 (18%) adalimumab a...
نمودار تعداد نتایج جستجو در هر سال
با کلیک روی نمودار نتایج را به سال انتشار فیلتر کنید