scholarly journals Slow Drift Solar Radio Bursts: Harmonic Frequency Ratios, Solar Longitude Dependence, and Frequency Drift Rates

1961 ◽  
Vol 14 (2) ◽  
pp. 234 ◽  
Author(s):  
Marion B Wood

Frequency ratios of second harmonic to fundamental bands are determined for 19 slow drift bursts. The ratios measured at the high frequency edges of the bands yield a mean value of 2� 00, whereas the mean value of the low frequency edge ratios is significantly lower than 2.

1974 ◽  
Vol 57 ◽  
pp. 291-292
Author(s):  
C. Caroubalos ◽  
M. Pick ◽  
C. Chiuderi ◽  
R. Giachetti ◽  
H. Rosenberg ◽  
...  

(Solar Phys.). The fine structure in solar type IV radio bursts was studied using the 169 MHz Nançay radioheliograph and the 60 channel radiospectrograph at Utrecht (160–320 MHz). The observed fine structure includes pulsating structure, zebra patterns (parallel drifting bands) and intermediate drift bursts. All are considered as modulation of high frequency radiation by low frequency oscillations or as the result of up conversion of low frequency oscillations to higher frequencies (Rosenberg, 1973).


Author(s):  
Vincent Libertiaux ◽  
William P. Seigfreid ◽  
Massimo A. Fazio ◽  
Juan F. Reynaud ◽  
Claude F. Burgoyne ◽  
...  

The optic nerve head (ONH) is the site of insult in glaucoma, the second leading cause of blindness worldwide. Intraocular pressure (IOP) is commonly regarded as a major factor in the onset and progression of the disease1 and lowering IOP is the only clinical treatment that has been shown to retard the onset and progression of glaucoma2. However, many patients continue to progress even at an epidemiologically-determined normal level of IOP3. This suggests that in addition to the mean value of IOP, IOP fluctuations could be a factor in glaucomatous pathophysiology. The importance of low frequency fluctuations of clinically-measured mean IOP remains controversial. These studies all rely on snapshot measurements of mean IOP at each time point, and those measurements are taken at relatively infrequent intervals (hourly at the most frequent, but usually monthly or longer). Recently however, there has been some interest in ocular pulse amplitude, or the fluctuation in IOP associated with the cardiac cycle, which can be measured by Dynamic Contour Tonometry (DCT). DCT provides continuous measurement of IOP, but only for a period of tens of seconds in which a patient can tolerate corneal contact without blinking or eye movement, which ironically are two of the most common sources of large high frequency IOP fluctuations according to our telemetric data collected from monkeys4 and previous human studies. In a recent report, continuous IOP telemetry was used in three nonhuman primates to characterize IOP dynamics at multiple time scales for multiple 24-hour periods5.


Author(s):  
Jamileh Fatahi ◽  
Maryam Amiri Jahromi ◽  
Fahimeh Hajiabolhassan ◽  
Amirsalar Jafarpisheh ◽  
Nariman Rahbar ◽  
...  

Background and Aim: The quick speech in noise (Q-SIN) test shows the difficulty of spee­ch perception in noise by specifying signal to noise ratio (SNR) loss. Although the Persian version of Q-SIN has been already constructed, the high-frequency emphasis version of this test is not available. The present study aimed to construct six lists with high-frequency emphasis and implement it. Methods: We are going to prepare a high-frequ­ency emphasis version of Q-SIN and then test it on a small sample. First, researchers designed the relevant sentences; then experts examined their content and face validity. According to the criteria for developing the Q-SIN test, six lists with high-frequency emphasis were prepared. The test was examined on 26 (13 male and 13 female), 18−35 years old individuals with nor­mal hearing. To determine the test reliability, it was re-administered three weeks later with the same conditions. Results: Of 76 sentences prepared, 36 sentences received enough credit after determination of their content and face validity. These 36 senten­ces were used to make 6 lists. The mean value of SNR50 in the Persian language was obtained -4 dB. The mean values of SNR loss in 6 lists were -1.65, -1.8, -2.23, -1.61, -2.38 and -2.07. The results showed equivalency of lists 1, 2, 3, 4, and 6. Examination of test-retest reliability indicated that all lists except the list 2were reliable. Conclusion: The lists of 1, 3, 4, and 6 are reli­able and equivalent and can be used in clinical application.


2002 ◽  
Vol 199 ◽  
pp. 488-489
Author(s):  
D. L. Jones

The GMRT represents a dramatic improvement in ground-based observing capabilities for low frequency radio astronomy. At sufficiently low frequencies, however, no ground-based facility will be able to produce high resolution images while looking through the ionosphere. A space-based array will be needed to explore the objects and processes which dominate the sky at the lowest radio frequencies. An imaging radio interferometer based on a large number of small, inexpensive satellites would be able to track solar radio bursts associated with coronal mass ejections out to the distance of Earth, determine the frequency and duration of early epochs of nonthermal activity in galaxies, and provide unique information about the interstellar medium.


2020 ◽  
Vol 143 (3) ◽  
Author(s):  
Goktug C. Ozmen ◽  
Mohsen Safaei ◽  
Lan Lan ◽  
Omer T. Inan

Abstract In this study, we propose a new mounting method to improve accelerometer sensing performance in the 50 Hz–10 kHz frequency band for knee sound measurement. The proposed method includes a thin double-sided adhesive tape for mounting and a 3D-printed custom-designed backing prototype. In our mechanical setup with an electrodynamic shaker, the measurements showed a 13 dB increase in the accelerometer's sensing performance in the 1–10 kHz frequency band when it is mounted with the craft tape under 2 N backing force applied through low-friction tape. As a proof-of-concept study, knee sounds of healthy subjects (n = 10) were recorded. When the backing force was applied, we observed statistically significant (p < 0.01) incremental changes in spectral centroid, spectral roll-off frequencies, and high-frequency (1–10 kHz) root-mean-square (RMS) acceleration, while low-frequency (50 Hz–1 kHz) RMS acceleration remained unchanged. The mean spectral centroid and spectral roll-off frequencies increased from 0.8 kHz and 4.15 kHz to 1.35 kHz and 5.9 kHz, respectively. The mean high-frequency acceleration increased from 0.45 mgRMS to 0.9 mgRMS with backing. We showed that the backing force improves the sensing performance of the accelerometer when mounted with the craft tape and the proposed backing prototype. This new method has the potential to be implemented in today's wearable systems to improve the sensing performance of accelerometers in knee sound measurements.


2020 ◽  
Vol 499 (1) ◽  
pp. 355-361 ◽  
Author(s):  
Wei-Yang Wang ◽  
Bing Zhang ◽  
Xuelei Chen ◽  
Renxin Xu

ABSTRACT Observations of the Faraday rotation measure, combined with the dispersion measure, can be used to infer the magnetoionic environment of a radio source. We investigate the magnetoionic environments of fast radio bursts (FRBs) by deriving their estimated average magnetic field strengths along the line of sight 〈B∥〉 in their host galaxies and comparing them with those of Galactic pulsars and magnetars. We find that for those FRBs with RM measurements, the mean 〈B∥〉 are $1.77^{+9.01}_{-1.48}\, \rm \mu G$ and $1.74^{+14.82}_{-1.55}\, \rm \mu G$ using two different methods, which is slightly larger but not inconsistent with the distribution of Galactic pulsars, $1.00^{+1.51}_{-0.60}\, \rm \mu G$. Only six Galactic magnetars have estimated 〈B∥〉. Excluding PSR J1745–2900 that has an anomalously high value due to its proximity with the Galactic Centre, the other five sources have a mean value of $1.70\, \rm \mu G$, which is statistically consistent with the 〈B∥〉 distributions of both Galactic pulsars and FRBs. There is no apparent trend of evolution of magnetar 〈B∥〉 as a function of age or surface magnetic field strength. Galactic pulsars and magnetars close to the Galactic Centre have relatively larger 〈B∥〉 values than other pulsars/magnetars. We discuss the implications of these results for the magnetoionic environments of FRB 121102 within the context of magnetar model and the model invoking a supermassive black hole, and for the origin of FRBs in general.


2009 ◽  
Vol 36 (3) ◽  
pp. 565-569 ◽  
Author(s):  
CAROLINA LLANOS ◽  
EDWARD K.L. CHAN ◽  
SONGQING LI ◽  
GRANT X. ABADAL ◽  
PETER IZMIRLY ◽  
...  

Objective.To evaluate the frequency of anti-α-enolase antibodies in the sera of mothers whose children have congenital heart block (CHB), given provocative results in which α-enolase, a membrane protein, was recognized by monoclonal antibodies reactive with the peptide p200 of 52 kDa Ro/SSA in a neonatal rat heart library.Methods.An ELISA using a recombinant α-enolase protein was developed. Sera from 100 anti-Ro52+ CHB mothers in the Research Registry for Neonatal Lupus, 50 patients with systemic lupus erythematosus (SLE; 7 anti-Ro52+), and 48 healthy controls were tested for anti-α-enolase reactivity.Results.There were no significant differences in the median values obtained from CHB mothers, patients with SLE, or controls at each of the dilutions tested. Only 7 (7%) at 1:100 dilution and 2 (2%) at 1:1000 dilution of 100 CHB sera were 3 standard deviations above the mean value obtained for controls. Preincubation with recombinant Ro52 did not inhibit anti-α-enolase reactivity.Conclusion.The low frequency of anti-α-enolase antibodies in the sera of CHB mothers and the absence of apparent cross-reactivity with Ro52 suggest that antibodies to Ro52 are not likely to mediate CHB via binding to α-enolase.


Blood ◽  
2005 ◽  
Vol 106 (11) ◽  
pp. 4904-4904
Author(s):  
Gina Zini ◽  
Mariagrazia Garzia ◽  
Antonella Di Mario ◽  
Bianca Maria Ricerca ◽  
Paola Piccioni ◽  
...  

Abstract The hematology analyzer Coulter LH750 provides WBC differential counts using the VCS technology, which combines three simultaneous measurements (Volume, Conductivity, Scatter) to classify circulating blood cells. Cell volume and internal cell structure (opacity) are detected, respectively, by applying a low frequency direct current (DC) and a high frequency alternative (RF) current. The light scattered at different angles between 10° and 70°, on the other hand, is proportional to cell size, granularity, surface topography and reflectance. The system also provides for the main four WBC subtypes (neutrophils, lymphocytes, monocytes, eosinophils) a set of data called ‘positional parameters’ (PP). They express the mean value and the standard deviation (SD) of the three VCS measurements. We focused our study to the analysis of PP of the neutrophil population in normal and in pathological samples in order to: i) evaluate any correspondence with morphology and ii) determine the predictivity of changes in these parameters for the presence of morphological abnormalities. We analysed 100 samples from healthy subjects, 59 males and 41 females, age ranged from 2 years to 79 years, (25 children, 75 adults) to define our neutrophil reference PP ranges. We found a mean volume of 151,7 (SD ± 22,5), a mean opacity of 143,9 (SD ± 7,4) and a mean scatter of 142,19 (SD ± 13,1), without consistent differences due to age or sex. Our results do agree with those found in the literature. In normal samples we could not observe, as expected, any morphological abnormality at the microscope. Thereafter we also analyzed 16 samples from patients with bacterial pneumonitis. Their PP showed a moderate increase in the mean volume (168,9 with SD ± 24,1), a normal value of opacity and a slight decrease of the mean scatter (138,2 with SD ±14.4). Microscope analysis showed granulocytes with normal morphology, sometimes with toxic granules and the presence of band forms and metamyelocytes above 7%. The analysis of the PP of 11 patients with chronic myeloid leukemia at diagnosis showed an increase in the mean volume (160,1) with a consistently highly SD (± 33,4); opacity (142,8 with SD ± 11,7) and scatter (143,9 with SD ± 12,3) were normal. At the microscope the morphology of neutrophils was normal, with the presence of circulating immature granulocytes (range 22–28%). Finally we analyzed samples from N 28 patients with myelodysplastic syndromes (14 RA, 5 RC, 9 RAEB Type 1). Circulating granulocytes showed a great increase in the mean volume with a wide dispersion (178,2 with SD ± 35,6 ), a decreased mean opacity (132 with SD ± 8,3) and very low mean scatter value (119,9 with SD ± 12,4). At microscope neutrophils showed characteristic dysplastic features, such as abnormal nuclear segmentation, chromatin clumping and hypogranularity. Our study demonstrates the Coulter LH750 PP are highly predictive of the presence of dysplastic neutrophils in the peripheral blood. We have found a peculiar data set (high volume with increased SD, low opacity and scatter with small SD) which is easily distinguishable from normal as well as from other types of neutrophil abnormalities, such as myloproliferative and bacterial diseases. These parameters are automatically available during the routine load of hematology laboratories and can be usefully utilized to screen and to early identify patients with mylodysplasia.


Sign in / Sign up

Export Citation Format

Share Document