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Giant Breast Involvement in Acute Lymphoblastic Leukemia: MRI Findings
Isil Basara,Sebnem Orguc 한국유방암학회 2012 Journal of breast cancer Vol.15 No.2
Breast metastases in cases of leukemia are rare. We aimed to report the conventional-advanced magnetic resonance imaging (MRI) findings of unilateral breast involvement of acute lymphoblastic leukemia (ALL) and review the literature. A 32-year-old woman was first diagnosed with ALL in treated in 2004. She did not continue the follow-up after 2008. She was presented with a giant, progressive right breast palpable mass in 2010. Mass,contralateral breast tissue were evaluated with MRI, diffusion weighted imaging and MR spectroscopy. With MRI findings, lesion was evaluated as malignant, tru-cut biopsy revealed recurrence of ALL. Lymphoma, malignant melanoma, rhabdomyosarcoma are most common tumors metastase to breast. Breast metastases of leukemia are rare and occur primarily in patients with acute myeloid leukemia. Secondary ALL breast involvement is uncommon. In a patient with malignancy, any enlarging breast mass, even with benign radiologic appearance, should be investigated carefully and metastasis should not be forgotten.
Aguilar, M.,Ali Cavasonza, L.,Alpat, B.,Ambrosi, G.,Arruda, L.,Attig, N.,Aupetit, S.,Azzarello, P.,Bachlechner, A.,Barao, F.,Barrau, A.,Barrin, L.,Bartoloni, A.,Basara, L.,Baş,eğ,mez-du Pree American Physical Society 2017 Physical Review Letters Vol.119 No.25
<P>We report the observation of new properties of primary cosmic rays He, C, and O measured in the rigidity (momentum/charge) range 2 GV to 3 TV with 90 x 10(6) helium, 8.4 x 10(6) carbon, and 7.0 x 10(6) oxygen nuclei collected by the Alpha Magnetic Spectrometer ( AMS) during the first five years of operation. Above 60 GV, these three spectra have identical rigidity dependence. They all deviate from a single power law above 200 GV and harden in an identical way.</P>
Aguilar, M.,Ali Cavasonza, L.,Ambrosi, G.,Arruda, L.,Attig, N.,Aupetit, S.,Azzarello, P.,Bachlechner, A.,Barao, F.,Barrau, A.,Barrin, L.,Bartoloni, A.,Basara, L.,Baş,eğ,mez-du Pree, S.,Batta American Physical Society 2016 Physical review letters Vol.117 No.23
<P>Knowledge of the rigidity dependence of the boron to carbon flux ratio (B/C) is important in understanding the propagation of cosmic rays. The precise measurement of the B/C ratio from 1.9 GV to 2.6 TV, based on 2.3 million boron and 8.3 million carbon nuclei collected by AMS during the first 5 years of operation, is presented. The detailed variation with rigidity of the B/C spectral index is reported for the first time. The B/C ratio does not show any significant structures in contrast to many cosmic ray models that require such structures at high rigidities. Remarkably, above 65 GV, the B/C ratio is well described by a single power law R. with index. Delta = -0.333 +/- 0.014(fit) +/- 0.005(syst), in good agreement with the Kolmogorov theory of turbulence which predicts. Delta = -1/3 asymptotically.</P>
Aguilar, M.,Ali Cavasonza, L.,Ambrosi, G.,Arruda, L.,Attig, N.,Aupetit, S.,Azzarello, P.,Bachlechner, A.,Barao, F.,Barrau, A.,Barrin, L.,Bartoloni, A.,Basara, L.,Baş,eğ,mez-du Pree, S.,Batta American Physical Society 2018 Physical Review Letters Vol.120 No.2
<P>We report on the observation of new properties of secondary cosmic rays Li, Be, and B measured in the rigidity (momentum per unit charge) range 1.9 GV to 3.3 TV with a total of 5.4 x 10(6) nuclei collected by AMS during the first five years of operation aboard the International Space Station. The Li and B fluxes have an identical rigidity dependence above 7 GV and all three fluxes have an identical rigidity dependence above 30 GV with the Li/Be flux ratio of 2.0 +/- 0.1. The three fluxes deviate from a single power law above 200 GV in an identical way. This behavior of secondary cosmic rays has also been observed in the AMS measurement of primary cosmic rays He, C, and O but the rigidity dependences of primary cosmic rays and of secondary cosmic rays are distinctly different. In particular, above 200 GV, the secondary cosmic rays harden more than the primary cosmic rays.</P>