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Morning Glory Disc Anomaly: Expanding the MR Phenotype.
F D Firouzabadi1,2, M D Soldatelli1, V Rameh1
1From the Department of Radiology (F.D.F., M.D.S. V.R., J.R., C.D.R.), Boston Children's Hospital and Harvard Medical School, Boston, Massachusetts.
AJNR. American Journal of Neuroradiology
|July 11, 2024
Summary
Morning glory disc anomaly (MGDA) often causes optic nerve thickening, potentially mimicking optic glioma. This condition is also frequently linked to persistent craniopharyngeal canals and other midline developmental abnormalities.
Area of Science:
- Ophthalmology
- Neuroradiology
- Pediatric Neurology
Background:
- Morning glory disc anomaly (MGDA) is a congenital condition affecting the optic disc.
- Imaging is crucial for identifying associated cephalocele and steno-occlusive vasculopathy.
Purpose of the Study:
- To assess optic nerve, chiasmatic, and sphenoid bone morphology in patients with MGDA.
- To evaluate potential misdiagnosis of optic glioma due to optic nerve thickening in MGDA.
Main Methods:
- Retrospective study of patients with funduscopically confirmed MGDA.
- Brain MRI imaging was used to evaluate optic nerve, chiasm, and sphenoid bone morphology.
Main Results:
- Thirty-two children with MGDA were analyzed.
- Ipsilateral optic nerve enlargement was common (21/32), potentially mimicking optic glioma.
- Associated findings included persistent craniopharyngeal canal (17/32), pituitary deformity (4/32), and nasopharyngeal lesions (10/32).
Conclusions:
- MGDA frequently presents with ipsilateral optic nerve thickening, posing a risk of misdiagnosis as optic glioma.
- MGDA is commonly associated with persistent craniopharyngeal canal, pituitary and infundibular deformities, cephalocele, and nasopharyngeal lesions.
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